The galaxy presents a largely featureless morphology, with a smooth and centrally concentrated light distribution. It appears elliptical in shape, though only slightly elongated. The galaxy's color gradient suggests a population of older stars, with a yellowish hue dominating the central bulge. There is no readily apparent evidence of spiral arms, dust lanes, or active star formation regions within the observed image. No indications of major gravitational disturbances or ongoing mergers are visible in this data. The overall appearance indicates a relatively evolved system, likely a quiescent elliptical galaxy.
