The galaxy presents as a primarily smooth, centrally concentrated object. The core exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. There is little evidence of distinct spiral arms or disk-like structure. The galaxy's overall shape appears to be somewhat elliptical, tending towards a rounded morphology rather than an elongated one. Faint, diffuse extensions or tidal features might be present, but are not sharply defined. The color gradients indicate a possible radial change in stellar populations. The overall appearance suggests a galaxy that is not undergoing major mergers or significant star formation at the present epoch.