The galaxy presents as a somewhat elongated, disk-like structure. It exhibits a prominent, centrally concentrated bulge that appears reddish in color, suggesting an older stellar population. Surrounding the bulge, a fainter, bluer disk is visible, indicating the presence of younger, hotter stars and potentially ongoing star formation. The disk appears relatively smooth, with no obvious spiral arm structure discernible at this resolution. The overall shape is somewhat cigar-like. There are hints of possible tidal disturbances or minor asymmetries in the outer regions of the disk, although no major merging activity is evident. The galaxy has a moderate redshift, placing it at a significant cosmological distance.
