The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical or lenticular, with a noticeable absence of strong spiral arm structures. A slight elongation is observed, but it is closer to round than cigar-shaped. The galaxy displays a gradient of light intensity that peaks at the core. The color profile is relatively uniform across the galaxy, suggesting a stellar population dominated by older stars and a relatively low rate of ongoing star formation. There is no evidence of a major ongoing merger, though the potential for minor tidal disturbance cannot be ruled out entirely. The overall impression is that of a fairly evolved galaxy, possibly in a state of relative quiescence with regards to star-forming activity.
