The galaxy presents an elongated morphology, appearing as a moderately disturbed system, possibly undergoing a minor merger or tidal interaction. There is an indication of a disk-like structure viewed at an oblique angle. The central region displays a smooth appearance with an amber hue, suggestive of an older stellar population. The presence of more intense colors, especially towards the center, points to an uneven distribution of stars and dust. The overall form is in between a cigar shape and circular. This morphology could be indicative of a galaxy undergoing a transformation in its structure due to internal dynamics or external interactions. There is also a very faint feature that could be a tidal tail.
