The galaxy presents an elliptical morphology, with a slightly elongated shape. It appears mostly smooth and undisturbed, lacking prominent spiral arms or a well-defined disk structure. The light distribution is concentrated towards the center, showing a bright core. There is a gradual fading of intensity as one moves away from the center. The color indices suggest a population of older stars, as it exhibits a redder hue. Star formation activity is low within the galaxy, which supports the conclusion of an older stellar population. The galaxy does not seem to be undergoing any major merging events. The overall impression is of a mature, relatively quiescent galaxy in a mid stage of its evolution.
