The galaxy exhibits a predominantly smooth morphology. It appears generally round, with a concentrated central bulge. The overall color profile suggests a population of older stars, indicated by the yellowish hue. There is a slight elongation, but the galaxy does not appear to be highly flattened. No distinct spiral arms or significant dust lanes are visible. There is no strong evidence of tidal disturbances or ongoing major mergers. The galaxy may be undergoing some minor interaction with another object.
