The galaxy appears as a single, relatively smooth object with a concentrated central region. It exhibits an elliptical morphology. The color profile suggests a population of older stars, contributing to the overall redder hue, with hints of bluer regions potentially indicating ongoing, albeit subdued, star formation. There are no readily discernible spiral arms or a prominent disk structure. There is no evidence of tidal features or other signs of recent or ongoing major mergers, although there may be a subtle distortion in its shape indicative of a minor interaction. The object's overall structure suggests a classification as an early-type galaxy with a mass characteristic of galaxies undergoing a moderate level of star formation.
