The galaxy presents as a centrally concentrated, elliptical or lenticular morphology. It exhibits a smooth light distribution, with no readily apparent spiral arms or prominent dust lanes visible in this image. The color profile indicates a yellow-to-red hue, suggesting an older stellar population with a relatively low rate of on-going star formation. There are no indications of major mergers or tidal disturbances present. The overall roundness suggests a minimal degree of flattening or elongation.
