The object presents as a relatively smooth, elliptical galaxy. Its overall color is indicative of a galaxy composed primarily of older stellar populations, emitting light mostly in the redder wavelengths. The galaxy exhibits a somewhat elongated morphology. There are no apparent spiral arms or significant dust lanes visible. The central bulge appears prominent and well-defined, contributing to the overall smooth appearance of the galaxy. There is no evidence of ongoing major mergers or tidal disturbances; the galaxy appears undisturbed. Its star formation rate is quite low. The morphology resembles a typical elliptical galaxy found within the local universe.
