The galaxy presents an overall elongated, cigar-shaped morphology. Its light is dominated by a central bulge that appears yellowish-white, suggesting a population of older stars. Fainter, bluish light emanates from the outer regions, possibly indicating areas of more recent star formation. A slight asymmetry or distortion can be observed. There seems to be a lack of well-defined spiral arms or other distinct structural features within the visible disk. Evidence suggests the possibility of minor gravitational interaction but is not a full on merger. 