The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. There is a slight elongation to the structure. Its color profile is dominated by redder hues, suggestive of an older stellar population and reduced recent star formation activity. The galaxy appears relatively undisturbed, lacking prominent spiral arms or irregular features typically associated with mergers or significant tidal interactions, though it is possible it is in the early stages of merging. There may be subtle irregularities in the light distribution that could point to some ongoing interaction or past merger event. I estimate it is a fairly massive system.
