The galaxy presents as a moderately luminous, relatively compact object. It appears to be largely smooth in texture, with a dominant central bulge exhibiting a yellow-orange hue, suggesting an older stellar population. There is a subtle transition outward, where the color shifts towards a slightly bluer tint, potentially indicative of ongoing or more recent star formation in the outer regions, however to a much lesser extent. The overall morphology is somewhat elliptical or lenticular, lacking prominent spiral arms or a well-defined disk structure. There is no obvious visual evidence of major disturbances or merging events. The galaxy appears relatively isolated and undisturbed within its immediate vicinity, presenting a quiescent appearance.
