The galaxy presents as a predominantly smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density. The overall color profile indicates a higher concentration of older stellar populations, with a yellowish hue dominating. There is a subtle asymmetry present, with a possible faint extension or tidal feature emanating from one side of the galaxy. This might suggest past or ongoing minor gravitational interaction with another nearby galaxy. There is little to no evidence of strong ongoing star formation, as indicated by the lack of prominent blue regions typically associated with younger, hotter stars.
