The galaxy appears to be a relatively smooth, disk-like structure with a pronounced central bulge. The color gradient suggests an older stellar population is dominant, exhibiting a yellowish-red hue overall. There's a slight elongation visible, indicating a possible oblate spheroid shape, tending toward being cigar shaped. There is little indication of any major disturbances or mergers. The overall morphology indicates a fairly evolved galaxy, with low levels of current star formation.
