The galaxy presents an overall elliptical morphology, appearing relatively smooth and concentrated towards its center. A significant bulge component is discernible, exhibiting a yellowish hue, suggestive of an older stellar population dominating the nuclear region. Fainter, bluer light extends from the core, possibly indicative of younger stars and some ongoing star formation. The galaxy appears to be undergoing some sort of gravitational disturbance or interaction, as its shape is not perfectly elliptical and there are some faint indications of tidal features or asymmetric light distribution. Overall, the galaxy gives the impression of being in an intermediate state of evolution, perhaps having undergone a past merger event and currently displaying characteristics between a quiescent elliptical and a more active spiral galaxy.
