The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round with a slight elongation. There are no visible spiral arms or a prominent disk-like structure. The color profile suggests an older stellar population, with a yellowish hue dominating the central region. Evidence of ongoing star formation is not readily apparent from visual inspection; the galaxy appears relatively quiescent. There is no indication of any major mergers or significant tidal disturbances; it seems relatively isolated and undisturbed. The galaxy’s overall appearance suggests it is a massive system with a high degree of spheroidal symmetry.
