The galaxy presents an elongated, disk-like morphology, suggesting a spiral or lenticular classification. The object displays a color gradient, appearing more yellow-red towards the central bulge and transitioning to a slightly bluer hue in the outer disk. This color difference may indicate varying stellar populations or dust content across the galactic structure, with younger, hotter stars possibly residing in the bluer regions. The galaxy exhibits a relatively smooth appearance with some features, the lack of obvious spiral arm structure or prominent dust lanes suggests that, if it is a spiral galaxy, it may be of a flocculent or weakly defined spiral arm type. Alternatively, the object could be an edge-on lenticular galaxy, lacking significant ongoing star formation. There is no obvious evidence of any major mergers or strong tidal disturbances.
