The galaxy appears to be a relatively smooth, elliptical-like system. It is centrally concentrated, exhibiting a radial gradient in surface brightness that decreases steadily outward from the core. The galaxy's overall shape is approximately round with no obvious signs of strong spiral arms, bars, or other major features associated with disk galaxies. There is a lack of any significant dust lanes or patchy regions of star formation visible. The galaxy's color suggests an older stellar population, being redder. There is no clear evidence of tidal disturbances, suggesting it is not currently undergoing a major merger. Overall, this galaxy appears to be a quiescent, early-type system.
