The galaxy presents as an elongated, cigar-shaped structure, with an apparent smooth morphology. The color gradient suggests a central concentration of older stellar populations, indicated by the yellow-ish core, fading into bluer regions towards the outer edges of the disk. This bluer coloration is potentially indicative of more recent or ongoing star formation. There is a slight asymmetry visible, possibly suggesting tidal interactions or minor disturbances. The overall light distribution appears relatively even and smooth, though closer inspection might reveal subtle features. The galaxy appears to be relatively quiescent, with a low star-formation rate. Given the galaxy's morphology and color profile, it may be classified as an early-type disk galaxy or potentially a lenticular galaxy undergoing transformation. There is no evidence of a major ongoing merger. 
