The galaxy presents as a smooth, elongated structure, with a high degree of axial ratio, indicative of an elliptical morphology viewed at a significant inclination. The central region exhibits a concentrated luminosity gradient, suggesting a prominent bulge. Color gradients are present, with the central bulge appearing more yellow/reddish, potentially due to an older stellar population or dust obscuration. The outer regions display a bluer hue, suggestive of more recent star formation, although it is not pronounced. There are no clear signs of spiral arms or strong dust lanes. Subtle irregularities in the light distribution hint at a possible minor disturbance or interaction, though the overall morphology is largely undisturbed. The galaxy appears relatively isolated.
