The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a concentrated, bright yellowish color, indicating a population of older stars. The galaxy's light profile appears to fade gradually outward from the center, with a redder hue, suggesting the potential for ongoing or recent star formation within the galaxy, though at a low rate. The lack of distinct spiral arms or other prominent features is consistent with an elliptical classification. There is slight asymmetry in the light distribution, hinting at a possible minor disturbance, potentially due to a past interaction or merger.
