The galaxy presents a morphology consistent with an elliptical type. It exhibits a generally smooth light distribution with a slight elongation along one axis, but is mostly round. There is little evidence of spiral arms or prominent dust lanes. The core region appears more concentrated and gradually diffuses outward into the halo. Color gradients indicate a redder hue in the central bulge, suggestive of an older stellar population. The outer regions display a subtly bluer tint, potentially indicating the presence of younger stars or a lower metallicity. Overall, the galaxy does not show signs of significant ongoing star formation or recent mergers, and is likely a relatively evolved system. No tidal tails or other signs of significant gravitational interaction are visible in the image.
