The galaxy presents as a moderately bright, somewhat elliptical structure. The central region appears as a luminous, diffused glow, suggesting a high concentration of older stars. The color is generally yellowish-white, consistent with a stellar population that is not dominated by young, hot stars. There is a noticeable lack of distinct spiral arms or dust lanes, which supports its classification as a galaxy with a relatively smooth appearance. Faint hints of bluer regions are present, implying a small amount of ongoing star formation. Overall, the galaxy has a well-defined, though somewhat diffuse, appearance, indicative of an evolved system. There are multiple other objects in apparent proximity which may or may not be physically related to this system, implying a galaxy group of some kind.
