The galaxy presents as a somewhat diffuse object with an overall elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a significant stellar density or potentially an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases. A plume-like extension is observed emanating from the central region. The plume displays a bluer hue, suggestive of a younger stellar population, and is indicative of a potential tidal interaction or ongoing star formation. The bulk of the galaxy appears yellowish-red which indicates an older stellar population. Based on the plume feature, there are signs of a possible minor merging event with a possible smaller galaxy nearby.
