This galaxy appears to be an elliptical galaxy, characterized by its smooth, featureless morphology. It presents a concentrated, centrally bright structure, with a radial decrease in luminosity. The shape appears more or less circular, showing only a slight deviation from perfect roundness. The overall color profile suggests a population of older stars, exhibiting a yellowish hue characteristic of such stellar populations. There is no readily apparent evidence of ongoing merging activity or significant tidal disturbances. Given the general lack of substructure, spiral arms, or prominent dust lanes, the galaxy likely has a low star formation rate.
