The galaxy appears to be a relatively smooth, elliptical system. The light profile suggests a high degree of central concentration, with a bright, yellowish core that gradually fades towards the outer edges. There is no distinct spiral arm structure or significant dust lane visible. The overall shape is generally round, with only a slight elongation. There are no obvious signs of ongoing major merger activity or significant tidal disturbances affecting the galaxy's structure. The light distribution is indicative of a stellar population dominated by older stars.
