The galaxy presents as a flattened, disc-like structure with a noticeable central bulge. There is evidence of a disc component exhibiting some spiral structure, though it is not highly defined. A significant fraction of the galaxy's light emanates from the central region, which appears smoother and more concentrated. The color profile suggests a mix of stellar populations, with the central regions trending towards redder hues, potentially indicating older stars or dust obscuration, while the outer disc shows bluer tints that suggest ongoing or recent star formation. Some morphological disturbance is indicated by an asymmetry in the distribution of light in the outer regions of the disc, especially on the left side of the image, possibly suggestive of a tidal interaction or minor merger. This galaxy is not perfectly symmetrical, having an elongated, cigar-like shape. 
