The galaxy presents as a somewhat elliptical, though relatively round, structure. Its core region exhibits a higher concentration of light, appearing brighter than its outer regions. The overall color profile suggests the presence of a mix of stellar populations; the central area has a subtle blue hue, possibly indicating recent star formation. A faint, diffuse disk is visible, appearing slightly warped on one side. The galaxy lacks well-defined spiral arms, suggesting it may be an early-type spiral or a lenticular galaxy. There is some subtle evidence of tidal disturbance, indicating a possible past interaction with another galaxy, though it's hard to tell.