The galaxy presents as a slightly elongated, disk-like structure seen at an oblique angle, nearing edge-on. The central bulge appears luminous with a yellow-orange hue, suggesting an older stellar population. The outer disk is less defined, exhibiting a bluer tint, potentially indicative of ongoing star formation. Faint, diffuse extensions are observable beyond the main body of the galaxy, hinting at tidal interactions or extended stellar halos. A slight asymmetry in the disk structure is noted, possibly the result of a minor disturbance or past merger event. The galaxy appears relatively smooth, with only subtle indications of spiral arm structures or prominent dust lanes. Overall, the galaxy displays characteristics of a late-type spiral or an early-type lenticular galaxy transitioning towards a more quiescent state.
