The galaxy presents as an elliptical morphology, appearing largely featureless and smooth in its light distribution. Its color is notably redder, with a concentration toward the center, suggesting a population of older stars dominating the stellar content. The shape is more in-between than perfectly round or cigar-shaped. There is no obvious indication of strong active galactic nucleus activity or significant ongoing star formation within the visible spectrum. The galaxy doesn't appear to be undergoing any major merging activity.
