The galaxy presents as a largely smooth, elliptical-like structure with a bright, concentrated core exhibiting a yellowish-orange hue. The overall shape appears elongated, though not severely so, with the light distribution gradually decreasing from the core outwards. There is little evidence of significant spiral arm structure or distinct features suggesting active star formation regions. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances, although there might be minor asymmetries in the outer regions indicating a past interaction. The galaxy exhibits colors consistent with an older stellar population.
