The galaxy appears as a centrally concentrated object with a relatively smooth, diffuse morphology. The light is brightest and most concentrated in the central region, suggesting a prominent galactic nucleus or bulge. The galaxy exhibits a color gradient, with a yellowish-white hue dominating the core and a slightly bluer, fainter light extending outward. The outer regions appear somewhat disturbed or irregular, possibly indicating tidal interactions or recent accretion events. Overall, the galaxy presents as a moderately luminous system with a mix of evolved stellar populations in the core and potentially ongoing star formation in the outer regions. A general round shape is visible, although the outer edges appear somewhat disrupted. No clear spiral arm structure is discernible, pointing toward an elliptical or lenticular classification, possibly experiencing minor gravitational interactions.
