The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting a high degree of roundness. There is a lack of obvious spiral arm structure or prominent dust lanes, suggesting a classification towards the elliptical end of the Hubble sequence. The galaxy's color is moderately red, indicating a population dominated by older stars and a reduced rate of ongoing star formation. There's no evident tidal disruption or major morphological abnormalities, indicating no recent major merger events, though minor disturbances cannot be ruled out. The overall appearance points towards a massive galaxy with a substantial stellar mass.
