The galaxy presents a generally smooth, elliptical morphology. The galaxy is concentrated, with light diminishing gradually from the central region outward. The core appears a yellow-white hue, indicating an older stellar population, potentially dominated by evolved stars. The outer regions exhibit a slight blue tinge, indicating the presence of some younger stars, although the overall star formation rate appears low. No distinct spiral arms or prominent dust lanes are visible. There is no indication of tidal disturbances or ongoing major mergers, suggesting it's a relatively isolated system. The light distribution is largely symmetrical, supporting the elliptical classification. The galaxy appears to be a quiescent system with a moderate mass and low ongoing star formation activity.
