The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light is distributed in a roughly circular pattern, showing no obvious spiral arm structures or significant disk-like features. The color profile indicates a population of older stars, with a subtle yellow-red hue dominating the core and extending throughout the galaxy. There are no apparent signs of ongoing major mergers or significant tidal disturbances, though a possible minor asymmetry might be present in its outer regions. The overall appearance suggests a spheroid-dominated system, potentially an elliptical galaxy or a lenticular galaxy with a dominant bulge.
