The galaxy presents as an elliptical structure with a high degree of elongation. Its primary axis is oriented approximately along a Northwest to Southeast direction. The central region exhibits a significantly higher surface brightness, appearing almost stellar in its intensity, and suggesting a concentrated nucleus. The color appears relatively uniform throughout the galaxy, trending toward a slightly blueish-white hue. The outer regions fade gradually, lacking any distinct features such as spiral arms or prominent dust lanes. The smooth morphology suggests a relatively quiescent system, potentially a spheroidal galaxy with minimal ongoing star formation. There is no visible evidence of mergers or tidal disturbances in the immediate vicinity of the galaxy, which is consistent with it being in a relatively stable state.
