The galaxy presents as a single, relatively smooth object with a concentrated central region. It exhibits a generally elliptical morphology, appearing largely spheroidal but with some deviation from perfect circularity. The color profile suggests a population of older stars, indicated by the reddish-gold hue, more pronounced towards the core. There is no strong evidence of spiral arm structure or significant dust lanes within this image. The overall light distribution decreases smoothly from the center outwards, consistent with an early-type galaxy classification, potentially an elliptical galaxy. There are no prominent tidal features or other signs of recent major mergers visible, though a slight asymmetry in the light distribution could indicate a past minor interaction.
