The galaxy presents as a centrally concentrated object, likely elliptical in morphology. There appears to be a smooth, diffuse halo surrounding a bright core. Color gradients are subtle but noticeable; the central region exhibits a yellowish-white hue, potentially indicating an older stellar population. Fainter, bluish tones are present in the outer regions suggesting the presence of younger, hotter stars, though these are not as pronounced as would be expected in a spiral galaxy with active star formation. There are no obvious signs of spiral arms or a distinct disk. No significant morphological disturbances or tidal features are discernible, suggesting it is unlikely to be undergoing a major merger event. The overall appearance is consistent with a relatively evolved galaxy with a moderate amount of ongoing star formation.
