The galaxy presents as a slightly elongated, disk-like structure viewed at a high inclination, close to edge-on. A prominent central bulge dominates the core, exhibiting a yellowish-orange hue suggesting a population of older stars. The disk component appears relatively smooth, with a subtle color gradient transitioning from the central bulge to a bluer tint at the periphery. This color shift may indicate regions of recent or ongoing star formation in the outer parts of the disk. The galaxy does not show evidence of strong spiral arm structure or significant dust lanes. There appears to be a faint, diffuse component extending slightly beyond the main body of the galaxy, possibly a stellar halo or tidal features. The overall morphology suggests a relatively evolved system, perhaps a late-type spiral or lenticular galaxy.
