The galaxy presents as a singular, relatively smooth, and centralized concentration of light. It exhibits an elliptical morphology, though not perfectly round, showing a slight elongation. The central bulge appears prominent, suggesting a high concentration of older stellar populations. The color is predominantly yellowish-orange, indicative of a galaxy dominated by older, redder stars. There is a lack of any distinct spiral arm structures or significant dust lanes. Marginal irregularities are present, potentially hinting at minor gravitational disturbances or interactions. The galaxy appears to be fairly quiescent in its star formation activity, as inferred from the color and overall smooth appearance.
