The galaxy presents as a relatively smooth, centrally concentrated object. It has an elliptical morphology, appearing somewhat cigar-shaped along its major axis. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or potentially an active galactic nucleus. The outer regions are less defined, with a gradual decrease in luminosity from the center outwards. Faint, diffuse extensions are visible along the major axis, hinting at possible tidal interactions or past merger events. The overall color index suggests a population dominated by older stars. There is a notable absence of distinct spiral arm structures or prominent star-forming regions, further supporting an older stellar population with a relatively low ongoing star formation rate. There appears to be some evidence of minor disturbance to its smooth structure.
