The galaxy presents a generally elliptical morphology. Its core exhibits high luminosity, indicating a significant concentration of stars. Moving outward from the central region, the luminosity gradually decreases. The overall color profile suggests an older stellar population with a dominant yellow-orange hue. There is some evidence of blue light in the outer regions of the disk, but these are not well defined. No obvious spiral arm structures or dust lanes are apparent, and the galaxy appears largely undisturbed. The galaxy appears to be relatively isolated with no nearby companion galaxies. Overall the galaxy is a mostly smooth, rounded object.
