This galaxy presents as a spiral, observed at a slight angle. The spiral arms are not tightly wound, with a moderately loose structure. A bulge is discernible at the center, appearing neither overly dominant nor negligible, presenting a moderate size. The overall color profile exhibits a range, with the central bulge appearing more yellow or golden, indicative of an older stellar population. Hints of blue can be seen within the spiral arms, suggesting ongoing star formation. There is no strong visual evidence of a bar structure crossing the central bulge. The spiral arms display a relatively symmetric pattern, most likely with two dominant arms. No extreme distortions are immediately obvious, however, slight disturbances and asymmetries may be present, potentially indicating minor gravitational interactions or internal dynamics. The galaxy appears to be undergoing active star formation, as indicated by the blue hues within the spiral arms. The galaxy is not currently undergoing a major merger, although it is possible it is undergoing a minor merging event.
