The galaxy presents an overall elliptical morphology, appearing smooth and relatively featureless. It exhibits a concentrated central region, suggesting a bulge-dominated structure. The light distribution gradually decreases outward from the center, with no distinct spiral arm features visible. There appears to be a faint asymmetry in the galaxy's overall shape, possibly indicating a past merger event or tidal interaction. The color profile indicates a population of older stars, consistent with a passively evolving system. The apparent extent of the galaxy is modest, indicating it is a typical galaxy. There appears to be a plume or tidal tail extending outward, further suggesting a possible gravitational interaction.
