The galaxy presents a largely smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in luminosity extending outwards from the core. The core region exhibits a yellow-orange hue, suggesting an older stellar population. The outer regions of the galaxy are less defined, fading into the background sky. There is a slight asymmetry visible in the light distribution, possibly indicating minor gravitational interactions or internal structures. No distinct spiral arms or bar features are discernible. The overall shape approximates a spheroid, with a moderate ellipticity. The galaxy exhibits no strong signs of tidal tails, bridges, or other indications of a major merger event, although there may be a faint distortion in its outer halo.
