The galaxy presents as a relatively compact object. Its morphology is predominantly smooth, with a slight elongation. The light distribution appears centrally concentrated. There is a subtle hint of structure, possibly a faint, disturbed disk, which contributes to the deviation from a perfectly elliptical shape. The color profile is fairly uniform, with no significant indication of distinct color gradients or prominent star-forming regions, which implies a relatively passive star formation rate. The galaxy shows some signs of gravitational disturbance, with a merging event with a smaller galaxy seeming likely.
