The galaxy presents as a centrally concentrated, elliptical morphology. The light profile appears smooth, with no obvious spiral arm structure or bar. The core exhibits a bright, compact appearance, suggesting a relatively high stellar density or potential AGN activity. The galaxy's color is generally yellowish-red, implying an older stellar population with a dominance of red giant stars and a relative lack of ongoing star formation. There's a very faint hint of an extended halo, possibly from tidal stripping, though further analysis would be needed to confirm this. The overall shape is highly circular. No significant dust lanes or signs of recent mergers are readily apparent.
