The galaxy exhibits a generally elongated, cigar-shaped morphology. It presents a smooth appearance with no clearly defined spiral arms or bar structure. There is a slight color gradient across the galaxy, with the central region appearing somewhat bluer than the outer regions. This suggests that the central region may be more actively forming stars compared to the edges. There are no obvious signs of a major ongoing merger, although there could be minor disturbances in the galaxy's morphology that require higher resolution imaging to confirm. The overall structure of the galaxy implies that it is likely an elliptical galaxy with a relatively low star formation rate.
