The galaxy presents as a lenticular or possibly an edge-on spiral galaxy, characterized by a bright, elliptical central bulge that dominates its overall morphology. The light from the bulge appears smooth and concentrated. Extending outwards from the central bulge, a faint, flattened disk is observed. This disk exhibits a subtle color gradient, transitioning from bluish hues in the outer regions to a more yellowish-white closer to the bulge, suggestive of variations in stellar populations. The disk structure lacks any distinct spiral arm features or prominent dust lanes, which supports the hypothesis that this is a lenticular galaxy, although the angle of observation makes it difficult to say with certainty. The overall shape is elongated, with a high aspect ratio implying a relatively thin disk when viewed edge-on. There appears to be some minor asymmetry in the disk's outer edges, though it is unclear if this is due to internal dynamics or tidal interactions.
