The galaxy presents as a compact, elliptical-like structure, exhibiting a smooth morphology with no discernible spiral arms or bar features. The light distribution appears relatively uniform across the galaxy, with a concentrated central bulge that gradually fades into the outer regions. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue. There is no apparent dust lane or any sign of active star formation regions. The galaxy displays a round appearance, suggesting a classification leaning towards an E0-E3 on the Hubble sequence. No signs of tidal disturbances or ongoing mergers are visible, indicating that it is a relaxed system.
