The galaxy appears as a relatively compact, centrally concentrated object. The overall morphology suggests a spheroidal shape, possibly elliptical, with a noticeable lack of distinct spiral arm structure. A subtle reddish hue is observed, indicative of an older stellar population and/or significant dust extinction. There's a slight asymmetry in its light distribution, hinting at possible tidal disturbances or recent minor merger events. Within the central region, there are hints of brighter, possibly younger stellar populations, but they are not sharply defined. The galaxy presents a rather smooth appearance, with no strong evidence of ongoing, large-scale star formation activity.
