The galaxy exhibits a generally smooth morphology, with a dominant, centrally concentrated bulge component. The galaxy appears largely elliptical in shape, trending towards round, but with a subtle elongation. There is a suggestion of faint, diffuse outer features or tidal disturbances, which could indicate past or ongoing interactions or minor mergers. The galaxy appears to be composed of an older stellar population due to its reddish hue. Evidence exists for some degree of disturbance, possibly the result of a minor interaction. There is also a possible sign of a recent merger or some other type of feature that has disrupted the typical smooth look.
