The galaxy presents as a relatively smooth, elongated structure, likely a disk galaxy viewed at an angle. A concentrated, bright central bulge is observed, displaying a yellowish hue indicative of an older stellar population. The disk appears somewhat diffuse with a bluer tint, which may indicate more recent star formation, though the star formation rate is estimated to be low. The galaxy shows minimal signs of major disturbances or mergers, although there may be some minor tidal features present or evidence of past interaction due to the slight asymmetry in the disk. The overall morphology is between round and cigar shaped.
