The galaxy presents as a relatively smooth, elliptical morphology. The primary body exhibits a cigar-like shape. There is no strong indication of significant star formation regions discernible at this resolution. The galaxy appears to be a relatively isolated system with no apparent major merging activity or tidal disturbances. The overall color gradient suggests a possible population of older stars, but with some signs of some younger stars as well. The object could potentially have a weak active galactic nucleus.
