The galaxy presents as a relatively smooth, elliptical object with a moderate degree of elongation. Its core region exhibits a concentrated luminosity, transitioning gradually outwards to a less intense halo. The color profile suggests a dominant population of older stars, indicated by the redder hues in the outer regions, which gradually shift towards a more yellow-white color at the galactic center. There is no apparent spiral structure or significant dust lane obscuration. The general form implies an evolved system, potentially an elliptical galaxy that has undergone significant merging or has ceased significant star formation activity. Possible minor tidal disturbances are present, suggesting a potential interaction with a dwarf galaxy or past galactic merger event.