The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of central concentration. The color profile suggests a population dominated by older stars, potentially with a low rate of on-going star formation. There is no discernable spiral arm structure or prominent dust lanes visible, nor is there apparent evidence of major interaction or recent merger activity. The general shape appears somewhat rounded, with no significant elongation or bar structure detected. Subtle asymmetry may be present, warranting further investigation of minor disturbances to the galactic structure.
