The galaxy appears as an elliptical morphology, with a smooth light distribution indicating a lack of prominent spiral arms or significant dust lanes. The core exhibits a concentrated, bright yellowish-white hue, suggesting a population of older stars. The galaxy's overall color profile transitions gradually from the yellowish core to a fainter, redder halo, indicative of an aging stellar population further from the nucleus. There is some subtle bluer light toward the outer edges of the galaxy. Overall, the galaxy shows a lack of current star forming activity with an old stellar population. There appears to be no significant signs of tidal disturbances or ongoing major mergers. The galaxy's structure is primarily spheroid, with no notable disk features.
