The galaxy presents as an elongated structure, approximately 6 kpc in effective radius. The light profile suggests it is not perfectly smooth, but possesses some degree of central concentration. The overall color is slightly yellow, suggestive of an older stellar population. There is a slight disk component of stars that can be visually identified. The color also indicates moderate star formation is present. There does appear to be some evidence of a minor disturbance in its morphology, although major merging activity cannot be ruled out. The galaxy's shape leans towards a cigar-like appearance when considering its elongation.
