The galaxy presents as a relatively smooth, disk-like structure, with a noticeable central bulge. The orientation is such that it is viewed at an angle, appearing somewhat elongated, but is in between round and cigar shaped. There is a color gradient visible, with the central region exhibiting a warmer, yellowish hue, possibly indicating an older stellar population or dust concentration. Progressing outwards from the center, a cooler, greenish tint is observed, suggesting the presence of younger stars or active star formation in the outer regions. No significant spiral arm structure or major disturbances are immediately apparent, and the overall form suggests a relatively undisturbed system, with only minor disturbances if anything.
