The galaxy presents an overall elliptical morphology, appearing as a flattened spheroid. A bright, concentrated nucleus is evident, suggesting a significant concentration of older stars in the galactic center. A disk structure is present, with regions of bluer hues indicating areas of ongoing star formation, particularly at the galactic edges. These regions contain younger, hotter stars. The disk appears somewhat disturbed or irregular, potentially influenced by past interactions. There is a faint hint of tidal features, suggesting minor gravitational disturbance or possible minor merging event, but the bulk of the light is concentrated in the central bulge and disk. The galaxy appears to be relatively massive with ongoing star formation activity.
