The galaxy presents as a largely smooth, disk-like structure with a concentrated central bulge. The object exhibits an elliptical shape, appearing elongated rather than perfectly circular.  There is a color gradient visible, transitioning from a central, yellowish-orange hue to a bluer color in the outer regions of the disk. This might suggest a difference in stellar populations or dust content between the bulge and the disk, with the bulge possibly containing older, redder stars and the disk harboring younger, bluer stars or a higher concentration of dust.

The overall morphology does not indicate any significant merging activity or major disturbances.  Faint, diffuse arms may be present, but are not well-defined. The galaxy's structure appears relatively undisturbed, suggesting a lack of recent major interactions with other galaxies. The smooth appearance indicates a high probability that the object is an elliptical galaxy, likely with minimal current star formation occurring within the bulge, but more active in the disk. The elliptical shape indicates that the object is not being viewed face on, but from an angle.
