The galaxy presents as a relatively smooth, elliptical morphology. It appears to be a single, consolidated object without prominent spiral arms or bar structures. The light distribution suggests a centrally concentrated luminosity profile, with the brightest region located near the center of the galaxy, gradually fading outwards.

The galaxy appears slightly elongated. The primary color is yellowish/orange, suggesting a population of older stars and a lower rate of on-going star formation. There are no distinct blue regions indicative of recent star formation. There are no visible signs of tidal disturbances, strong gravitational lensing effects, or interactions with other galaxies. The smoothness of the light distribution and lack of visible substructure suggest that the galaxy has likely undergone significant dynamical relaxation.
