The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The overall shape appears somewhat rounded, transitioning from a circular to a slightly elliptical form. The light profile suggests a single, dominant component, lacking discernible spiral arms or a distinct bar structure. The galaxy exhibits a color gradient, appearing bluer toward the core and becoming progressively redder in the outer regions, indicative of differing stellar populations and ages. There are no obvious signs of tidal disturbances, major mergers, or significant ongoing star formation. A subtle, minor asymmetry might be present, but it's not strong enough to suggest a major interaction. Overall, this galaxy appears to be an evolved system, possibly an elliptical or lenticular galaxy with a substantial population of older stars.
