The galaxy appears as a single, largely featureless object, exhibiting a smooth, elliptical morphology. It has a concentrated central bulge that is a bright yellowish-orange hue. The light gradually decreases in intensity with distance from the center, creating a diffuse halo. There is a lack of any obvious spiral arm structure or dust lanes. The galaxy shows a general roundness rather than a flattened disc shape. There are no readily apparent signs of ongoing major mergers or significant tidal disturbances, though minor distortions might be present upon closer inspection. The color profile suggests a stellar population dominated by older stars.
