The galaxy presents a generally smooth and rounded morphology. A concentrated central bulge appears dominant, displaying a yellowish-orange hue suggestive of an older stellar population. A faint, slightly bluer halo surrounds the bulge, implying the presence of some younger stars or ongoing star formation within the galaxy. There is a subtle indication of some minor disturbances in the outer regions of the galaxy, with possibly some faint tidal features present. These disturbances could possibly result from a past or ongoing interaction with another galaxy. The overall impression is of an evolved galaxy with a dominant spheroidal component, experiencing a low level of star formation activity.
