The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing more elongated than perfectly spherical. The central region is brighter and more diffuse, indicative of a bulge component. There is a slight bluing trend in the galaxy's color, suggesting some degree of ongoing star formation, though it does not appear to be a strongly star-forming system. Faint disturbances in the galaxy's outer halo suggest possible minor interaction or merging event in its past. Overall, the galaxy appears to be a mature system undergoing only moderate stellar evolution.
