The galaxy presents as a somewhat elongated structure with a prominent central bulge that gradually fades into a less defined disk. The color profile suggests an older stellar population dominates, particularly in the central region, as indicated by the redder hues concentrated there. A faint bluish tint is observed in the outer regions of the disk, potentially indicative of more recent star formation activity, though it appears to be subdued. The galaxy exhibits a relatively smooth morphology, with no apparent spiral arms or significant dust lanes. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The shape is more rounded than cigar shaped.