The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits an elliptical or lenticular morphology, appearing mostly round in shape, with only a slight elongation. A bright central bulge is observed, surrounded by a fainter, more diffuse halo or disk. Subtle color gradients are visible; the central bulge has a yellowish or orange hue, suggesting an older stellar population, while the outer regions show a faint bluish tinge, potentially indicating the presence of younger, hotter stars or ongoing star formation in these areas. There is no apparent evidence of strong spiral arm structure or significant dust lanes. Possible minor disturbances appear to be present, though no major merging activity is evident.
