The galaxy appears to be a relatively faint, elongated structure, exhibiting a somewhat cigar-shaped morphology. A slight redder hue is noticeable in the central region, potentially indicating an older stellar population or dust obscuration. The disk component is faint, yet subtly visible, with only hints of spiral structure discernible. The galaxy shows no signs of intense star formation. The overall smooth appearance suggests a limited amount of ongoing major mergers or significant tidal disturbances.
