The galaxy presents as a somewhat faint, elongated structure with a moderately inclined disk. The color profile suggests a mix of stellar populations, with a slightly bluer hue concentrated towards the central regions, potentially indicative of ongoing star formation. Dust lanes may be present, contributing to the patchy and somewhat obscured appearance. The overall morphology suggests a spiral galaxy, although with some irregularities and a potentially disturbed structure, suggesting possible past interactions or mergers. The galaxy is not particularly luminous, based on its apparent magnitude, and the disk appears relatively smooth. There is no obvious central bulge. Overall, the galaxy appears to be a moderately sized, possibly actively star-forming spiral galaxy undergoing some level of interaction or disturbance.
