The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth and featureless morphology. The core region displays a bright, yellowish-white hue, suggesting a high concentration of older stellar populations and potentially a significant bulge component. A faint, diffuse halo extends outwards from the core, gradually fading into the background. The overall shape appears close to circular. Subtle hints of bluer light are present in the outer regions, possibly indicating ongoing or recent star formation, although this activity appears to be subdued. There is no obvious evidence of spiral arm structure or significant tidal disturbances.
