The galaxy presents as a single, centrally concentrated object with a relatively smooth morphology. The core region displays a bright, nearly uniform luminosity. The galaxy exhibits an elliptical shape, with the ratio of major to minor axis appearing nearly equal indicating that it is a close to face-on. The color profile suggests a population of primarily older stars, exhibiting a redder hue overall, with perhaps a hint of younger bluer stars in the disc. There are no distinct spiral arms, bars, or other significant morphological features visible. Based on these observations, the galaxy is likely a relatively massive early-type galaxy, possibly an elliptical or lenticular type. There is no visual evidence of ongoing major mergers or tidal disturbances.
