The galaxy presents as a relatively compact and luminous object. The overall morphology appears elliptical, lacking prominent spiral arms or a distinct disk structure. There is a smooth distribution of light, suggesting a dominant stellar population of older stars. The central region appears more concentrated, possibly indicating a bulge component. The color profile shows a broad range from a pale, whitish center, to a soft yellow and even a pale blue in the outermost ranges. The uniformity of the light distribution hints at a well-mixed stellar population within this galaxy. There is no readily apparent evidence of ongoing major merging events, but a slight asymmetry suggests the possibility of past or minor interactions.
