The galaxy presents a relatively smooth, elliptical morphology. It appears largely featureless with a diffuse central bulge that transitions gradually into the outer regions. The galaxy exhibits a color gradient, appearing slightly bluer in its outer edges compared to the yellower core region. This could indicate the presence of a younger stellar population residing in the disk or outer regions. There is a subtle asymmetry in the overall shape, suggesting a possible gravitational interaction or minor disturbance. No distinct spiral arms or significant dust lanes are apparent. Based on the estimated redshift, this galaxy is at an intermediate distance. The low estimated star formation rate suggests it may be a relatively quiescent galaxy.
