The galaxy appears to be a relatively smooth, elliptical system. Its light profile suggests a concentrated bulge, as indicated by the centralized bright region. The overall color is somewhat reddish-yellow, implying a population of older stars and a reduced rate of ongoing star formation. There is a slight elongation to the galaxy's shape, presenting a somewhat cigar-like appearance, but the system lacks any prominent spiral arm structures or significant dust lanes that would suggest a more disk-dominated morphology. There's no clear evidence of tidal features or major disturbances from ongoing mergers, although a slight asymmetry can be observed, suggesting a possible minor interaction in its past.
