The galaxy appears to be a relatively smooth, elliptical type. Its light is centrally concentrated, with a gradual decrease in surface brightness moving outwards. The core region displays a yellowish hue, suggestive of an older stellar population. No distinct spiral arms or prominent dust lanes are visible. The overall morphology indicates a well-defined, rounded shape, with only a very slight deviation from perfect circularity. There is no obvious sign of a recent merger event or significant tidal disturbance in the surrounding environment. The galaxy exhibits a general lack of blue light indicating a low star formation rate.
