The galaxy presents as a fairly smooth object, appearing somewhat elliptical in shape. A bright central bulge is noticeable, gradually fading into a less luminous disk. There may be faint disturbances hinting at minor interactions, though the overall structure remains largely undisturbed. The color distribution suggests a mix of stellar populations, with bluer hues concentrated in the central regions, possibly indicating ongoing or recent star formation. The outer regions appear redder, perhaps indicative of an older stellar population. The galaxy is well-defined, but lacks prominent spiral arms or other distinct features.
