The galaxy presents with an overall yellowish-orange hue, suggesting a dominant population of older stars. The light is relatively smooth and concentrated, implying a possible elliptical morphology or a spiral galaxy with a prominent bulge. Faint, somewhat irregular extensions are visible on one side, hinting at potential tidal features or ongoing interactions, and the possibility of some disturbed morphology. There is some indication of bluer light within the irregular extensions, potentially indicative of some star formation.
