The galaxy presents as a relatively smooth object with a somewhat elliptical morphology. It appears centrally condensed, with a gradual decline in surface brightness moving outward from the core. The color profile is generally uniform across the galaxy, leaning towards a yellow/orange hue. This suggests a stellar population dominated by older stars. There is no visible evidence of spiral arm structure or significant dust lanes. There appear to be no signs of significant tidal features or ongoing mergers, though there is some very minor indication of a potential disturbance in the form of slight asymmetry. The galaxy's overall appearance suggests that it is a fairly relaxed system.
