The galaxy presents a morphology that is neither purely elliptical nor fully spiral, exhibiting characteristics suggestive of a transitional form. The central region appears relatively smooth and concentrated, but there's evidence of a faint, disklike structure extending outward. The overall light distribution suggests that the galaxy may not be perfectly relaxed, and there might be ongoing or recent interactions. There is a slight asymmetry in the outer regions, with a small amount of tidal disturbance likely indicative of a gravitational interaction with another galaxy. The color suggests that star formation rate is low. Based on the apparent roundness, it appears to be viewed at close to face-on. The light profile is relatively smooth, without strong knots or regions of intense star formation visible.
