The galaxy presents an overall elliptical morphology, exhibiting a relatively smooth appearance in its central region. The light profile appears centrally concentrated, with a noticeable decrease in surface brightness moving outwards from the core. There is subtle evidence of a faint, extended halo surrounding the primary body of the galaxy. Close inspection reveals possible minor disturbances in the outer regions, potentially hinting at tidal interactions or recent accretion events. The color distribution indicates a generally older stellar population, characterized by yellowish hues. Star formation appears suppressed across the galaxy, correlating with the dominance of evolved stars. The galaxy does not show strong indications of spiral arms or a prominent disk structure.
