The galaxy presents as a moderately luminous object with an elliptical morphology, elongated along a principal axis. The central region exhibits a high degree of smoothness and a concentrated luminosity profile, indicative of an older stellar population. Fainter, less defined extensions are observed at the periphery of the galaxy along the major axis. There may be some evidence of minimal disturbances in the outer structure. Overall, the galaxy is well-defined, and there are no clear signs of significant ongoing mergers or tidal interactions. The overall color appears to be a somewhat redder hue.
