The galaxy presents a generally smooth morphology, with a somewhat elliptical shape. The light distribution appears concentrated toward the center, suggesting a possible bulge. It exhibits a color gradient, with the core appearing more yellowish-white, indicative of an older stellar population. A fainter, bluer region extends outwards from the core on one side, possibly suggesting the presence of younger stars or ongoing star formation in that area. There is no evidence of spiral arms or a well-defined disk structure. The overall structure does not show obvious signs of major mergers or significant tidal disturbances, though there seems to be a very minor light distortion nearby.
