The galaxy presents as a largely smooth, centrally concentrated object. It exhibits a fairly elliptical morphology, tending toward the "in between" classification of roundness. The galaxy is characterized by a prominent bulge that dominates the overall light profile, with colors appearing to shift to longer wavelengths towards the center. The disk, if present, is not well-resolved. There is no strong evidence of spiral arms or distinct features, with only minor indication of disturbances, such as tidal tails or merging activity. The color indices suggest a galaxy dominated by an older stellar population. Overall, this appears to be a fairly massive galaxy.
