The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge and lacks prominent spiral arm structures. The color appears predominantly yellow-red, suggesting a stellar population composed of older, redder stars. The galaxy's light profile is generally round, with a slight deviation toward a cigar shape. There is no evidence of any ongoing major merging activity; however, a minor disturbance cannot be excluded. The galaxy possesses a high stellar mass and a suppressed star formation rate. It has a redshift of approximately 0.19, indicating that it is at a considerable distance from our own galaxy.
