The galaxy presents a generally smooth, elliptical morphology. The light distribution is concentrated towards the center, showing a bright core. The galaxy appears roughly round in shape, with a slight elongation that is difficult to discern. There are no clearly defined spiral arms or a prominent disk structure evident. The light color is indicative of an older stellar population. The galaxy possibly exhibits signs of interaction or merger activity, though no substantial tidal tails or bridges are immediately obvious. Further investigation might reveal more subtle signatures.
