The galaxy presents as a single, dominant, centrally concentrated object. It appears largely elliptical in shape, with a smooth, relatively featureless morphology. There is a high degree of central concentration of light.

The color gradient suggests an older stellar population, appearing more luminous in the redder bands, with a decrease in luminosity toward bluer wavelengths. This is consistent with a galaxy that has undergone significant star formation in the past, which has since decreased, and now contains primarily older, redder stars. No obvious spiral arm structures are present, and there are no signs of ongoing major mergers or tidal disturbances. A slight irregularity on the edge of the galaxy indicates a possible minor interaction with another galaxy.
