The galaxy presents as an elliptical or lenticular type, exhibiting a relatively smooth, centralized light distribution. It displays a yellowish hue, suggestive of an older stellar population and minimal ongoing star formation. The overall shape is somewhat elongated, though the aspect ratio is closer to round than cigar-shaped. There's no clear evidence of spiral arms or strong dust lanes. A slight asymmetry is present; it could be a sign of a minor interaction with another galaxy or simply an irregular distribution of stellar density. Further spectroscopic data would be necessary to determine more precise details of its composition, dynamics, and evolutionary state.
