The galaxy presents as a relatively smooth, somewhat elongated structure. Its light profile suggests a possible early-type morphology, perhaps an elliptical or lenticular galaxy, given the lack of distinct spiral arms or prominent dust lanes. There is a slight elongation, with the galaxy appearing somewhat cigar-shaped. The dominant color is a yellowish-white hue, indicating a population of older stars. There is no obvious nucleus. There may be minor disturbances within the galaxy, but no signs of a major merger.
