The galaxy presents as a flattened, disk-like structure, elongated along a major axis. Its overall color appears to be a pale yellow-white, indicative of an older stellar population. A slight reddish hue is observed within the central bulge, potentially signaling the presence of dust obscuration or older, redder stars concentrated in that region. The disk appears relatively smooth with no clear spiral arm structure visible in this image. The morphology suggests the possibility of a galaxy undergoing a minor disturbance event, evidenced by some irregularities along its primary axis. There may be evidence of an ongoing or recent minor merger event, although it does not appear to be disrupting the overall structure significantly. The object's profile is best described as in between round and cigar shaped. 
