The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. There is a slight elongation, but the overall structure lacks prominent spiral arms or a well-defined disk. The light distribution is concentrated towards the center, with a gradual decrease in surface brightness towards the edges. The galaxy exhibits a color gradient, transitioning from a bluer core to yellower outer regions. There are some signs of possible tidal disturbances or faint asymmetric features, suggesting past minor merger or interaction events, although there is no obvious major merger. Overall, it seems to be a relatively old galaxy with a likely substantial stellar mass and a low rate of star formation.
