The galaxy presents as a relatively smooth, elongated object. Its color is predominantly yellowish-white, with the central region appearing brighter and more concentrated. This suggests an older stellar population is dominant towards the core. The overall shape approximates a cigar or elliptical form, with a significant length-to-width ratio. While there is a suggestion of a disk-like structure, it lacks prominent spiral arms or distinct features. Faint extensions or a subtle warp may be present along the major axis, hinting at possible interactions or past disturbances. The lack of clearly defined structure points toward the possibility of a galaxy undergoing morphological transformation or being dominated by a bulge component.
