The galaxy presents an elliptical morphology, exhibiting a concentrated, luminous core that gradually diffuses outwards. The galaxy appears relatively smooth, lacking prominent spiral arms or significant dust lanes. The central region displays a yellowish hue, possibly indicative of an older stellar population. Moving outward from the core, a bluer tint emerges, suggesting the presence of younger stars and ongoing, though likely limited, star formation. The overall shape is slightly elongated. The galaxy does not appear to be undergoing any major merging events or significant disturbances.
