The galaxy appears as a slightly elongated, diffuse object with a relatively smooth morphology. The light distribution suggests a concentrated central region that fades gradually outwards, indicating little to no spiral arm structure or prominent features such as dust lanes or star-forming regions. It presents an overall elliptical shape, being mostly in between round and cigar shaped. The color profile shows a slight reddening. The galaxy exhibits some evidence of a minor disturbance, but is not undergoing a major merger. The galaxy has a moderate to high stellar mass. It presents a moderate rate of star formation, but in comparison to its stellar mass, the specific star formation rate is low, suggesting that it is on the red sequence.
