The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular classification. There is a slight elongation, appearing cigar-shaped rather than perfectly round, and indicates possible ongoing or past interactions. A central bulge region is visible, exhibiting a yellowish hue which implies an older stellar population, while the outer regions appear fainter. No distinct spiral arm structures are discernible, reinforcing the assessment of a relatively featureless disk. The galaxy appears relatively isolated with no obvious tidal features or nearby companions immediately apparent in the image, though a minor disturbance is possible. Color variation is subtle, with a bluer tint near the edges, possibly indicating some ongoing star formation, though at a relatively low rate. Overall, it presents itself as a galaxy with a dominant smooth component and characteristics that are commonly seen in galaxies of moderate mass.
