The galaxy appears to be a relatively smooth, elliptical-type galaxy with a concentrated central bulge. There is a lack of discernible spiral arm structure or distinct features. The color profile suggests a population of older stars, with a dominant yellowish-red hue, gradually shifting towards a blue core, potentially indicating ongoing, or recent, star formation in the central region. There is no obvious sign of tidal disturbance or a major merger event, but there could be a minor interaction with another galaxy that cannot be seen from this image. The isophotes are generally regular and elliptical in shape.
