The galaxy appears as a concentrated, relatively smooth distribution of light. It exhibits a somewhat elliptical morphology, though tending towards roundness, with no distinct features such as spiral arms or a prominent bar visible at this resolution. There is a slight elongation, but it is not strongly cigar-shaped. The galaxy presents a consistent color profile, with a subtle shift toward redder hues, indicating the presence of older stellar populations. There is no strong evidence of ongoing major merging activity or significant tidal disturbances based on the morphology. The light is concentrated in the central region, indicative of an early-type galaxy or a late-type galaxy viewed at a large distance where spiral arms are less distinct.
