The galaxy appears as a somewhat diffuse, flattened structure with a moderate degree of central concentration. The color profile suggests a stellar population that includes both older, redder stars and a significant presence of younger, bluer stars indicative of ongoing or recent star formation. The galaxy exhibits a subtle asymmetry in its overall shape, hinting at potential interactions or internal dynamics. There is a faint suggestion of spiral arm structure, though it is not well-defined. A slight central bulge is present, though not particularly prominent. There is evidence of some dust lanes or patchy obscuration. Overall, it appears to be a relatively low-mass spiral or irregular galaxy undergoing moderate star formation.
