The galaxy presents as a primarily smooth, elliptical object, exhibiting a concentrated central bulge. Its color profile is distinctly redder than average, suggesting a population dominated by older stars and a lower rate of ongoing star formation. There are morphological irregularities suggestive of a recent or ongoing interaction or merger, with some visual indications of tidal features. The system shows signs of disturbance and a possible active galactic nuclei. The galaxy appears to have a considerable mass, which is consistent with the observed high luminosity.
