The galaxy presents as a single, concentrated light source with a smooth, elliptical morphology. It exhibits a fairly uniform yellowish-white color profile, suggesting a stellar population dominated by older, evolved stars. There is no apparent spiral structure, dust lanes, or active star-forming regions visible in this image. The light intensity decreases gradually from the center, without any abrupt changes or distinct features. The overall roundness of the galaxy is notable, with no significant elongation or tidal distortions observed. There is no sign of any ongoing or recent mergers.
