The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile suggests a dominant bulge component, appearing roughly elliptical in shape. There is a slight elongation, making it slightly 'in between' round and cigar-shaped. The color distribution indicates a possible redder core, shifting to bluer hues in the outer regions. No strong spiral arm structures or prominent dust lanes are immediately apparent. There may be a minor disturbance in its outer regions, but no indications of an ongoing major merger.
