This galaxy presents a relatively smooth, concentrated appearance, with a central bulge that dominates its overall light profile. The object is generally elliptical in shape, appearing mostly round when viewed from our vantage point. The is little evidence of spiral arm structures, but there are some notable hints of disturbances. These are most likely the result of some kind of interaction.

In terms of color, the core region exhibits bluer hues, indicative of a younger stellar population, while the outer regions trend towards redder colors, suggestive of older, cooler stars. The overall color profile suggests ongoing or recently quenched star formation activity, although the redder outer regions point to a population of older stars. There is no obvious sign of any major merging or tidal tails.
