The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The light profile is relatively even across the main body of the galaxy, suggesting a lack of significant spiral arm structure or prominent dust lanes. The color is yellowish-white, implying a relatively old stellar population with lower levels of ongoing star formation. It has a slightly elongated shape but is fairly round, resembling a flattened spheroid rather than a highly inclined disk. There is no visual evidence of a recent major merger or tidal disruption, and no obvious signs of strong active galactic nucleus activity or a bright central quasar. The galaxy is relatively compact, its overall size consistent with that of an elliptical or lenticular galaxy at its estimated distance.
