The galaxy presents as a relatively smooth, rounded structure. It appears to be an elliptical galaxy, lacking prominent spiral arms or a well-defined disk. There is little evidence of significant dust lanes or patchy star formation regions. The galaxy exhibits a concentrated central bulge that is strongly luminous. The color profile suggests a population of older stars. No significant tidal distortions or signs of an ongoing major merger are immediately apparent. The overall morphology indicates a system that is likely in a relatively quiescent state.
