The galaxy presents an overall smooth, elliptical morphology. It appears to be primarily spheroid in shape, with a length that is greater than its width giving it an cigar-shaped appearance. There is minimal evidence of spiral arm structure. The central region appears brighter and more concentrated than the outer edges, suggesting a higher density of stars and potentially a central supermassive black hole. The color is primarily blue, with traces of red at the edges, indicating the presence of a young star population. There are no obvious signs of a recent major merger, although there appears to be slight disturbances in the overall shape, possibly indicating a minor disturbance or interaction with a smaller galaxy in the past. The galaxy exhibits a low star formation rate, with minimal presence of HII regions. It appears to be an early-type galaxy undergoing a process of quenching star formation.
