The galaxy presents as an elongated, somewhat cigar-shaped structure. A smooth, centrally concentrated bulge dominates the light profile. There is evidence of a disk extending beyond this central bulge, although the disk appears largely featureless. Color gradients are apparent, with the central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions of the disk show a subtle shift towards bluer colors, indicating the presence of younger, hotter stars, although star formation appears to be relatively quiescent. There is no obvious evidence of spiral arm structure or significant dust lanes. The galaxy shows no signs of major mergers, tidal tails, or strong gravitational disturbances. It is likely a massive galaxy with a relatively high stellar mass and a low specific star formation rate.