The galaxy presents as a single, relatively smooth object with a concentrated central bulge. Its morphology appears elliptical, exhibiting a high degree of circularity with no apparent disk structure. Coloration suggests a population of older stars, as indicated by the yellowish-red hue. There is no evidence of active star formation regions, spiral arms, or significant dust lanes. The galaxy appears undisturbed, lacking tidal features or signs of recent merger activity. Overall, it appears to be a mature, quiescent galaxy.
