This galaxy appears to be a relatively smooth, elliptical system, exhibiting a spheroidal morphology. It displays a concentrated central bulge that dominates its overall luminosity profile. The galaxy's color index suggests a population of older stars, with a slightly redder hue concentrated towards the core, possibly indicating a greater density of evolved stars and/or dust. There is no obvious disk component or spiral arm structure visible in the image, supporting a classification as an elliptical galaxy. There are no signs of any ongoing major mergers or significant tidal disturbances, as the galaxy appears relatively undisturbed.
