The galaxy presents a largely smooth morphology, with a centrally concentrated luminosity profile. It appears elliptical in shape, exhibiting an elongated form with a high degree of axisymmetry. There is little evidence of spiral arm structure or significant dust lanes within the visible spectrum. The light distribution suggests a stellar population that is dominated by older stars, exhibiting an orangish-yellow hue. Faint, extended features are visible around the core, showing a lack of patchiness. It is likely a massive system with suppressed star formation activity. No significant tidal features are visible.
