The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated luminosity, appearing yellowish, indicative of an older stellar population. Surrounding the core, a more diffuse, bluish halo suggests the presence of younger, hotter stars and some ongoing, albeit modest, star formation activity. The galaxy does not display any prominent spiral arm structures or distinct dust lanes. The overall shape appears relatively round, with a slight elongation, not quite cigar shaped. There is no evidence of any major ongoing merger events, though subtle asymmetries and faint extensions may indicate minor tidal interactions or past disturbances.
