The galaxy presents a generally smooth appearance, with no immediately discernible spiral arm structure. The light distribution is concentrated toward the center, indicating a prominent bulge. The galaxy appears slightly elliptical in shape. The galaxy has a yellow hue in the central part, and it slowly fades to a faint pale color toward the edges. Based on its color and morphology, it is likely a galaxy containing a population of older stars, potentially indicating ongoing or recently quenched star formation. There is no evidence of active galactic nuclei features or strong tidal distortions. It is a relatively isolated object.
