The galaxy appears to be a relatively smooth, centrally concentrated object with a slight elongation. The central region is significantly brighter and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer regions are visible in the surrounding areas, potentially indicative of ongoing or recent star formation. There is no apparent spiral structure or strong dust lanes. A slight disturbance or faint tidal feature may be present, suggesting a past interaction with another galaxy. The overall morphology suggests this galaxy is likely an elliptical galaxy with a possible low level of star formation.
