The galaxy presents a generally elliptical morphology, with a smooth, centralized concentration of light. The core is bright and yellowish-white, suggesting a population of older stars. Moving outwards from the core, the light becomes more diffuse and the color appears slightly redder, indicative of a fainter distribution of similar stellar populations. There are no readily discernible spiral arms or dust lanes, implying a relatively featureless, well-mixed structure. The overall color profile suggests a galaxy with a predominantly older stellar population and little ongoing star formation. The shape appears to be only slightly elongated, trending towards round, with no apparent major disturbances or signs of recent merger activity.