This galaxy presents as a slightly inclined spiral, viewed at an angle that reveals a flattened disk structure. The central bulge is prominent, displaying a concentrated, yellowish hue, suggesting a population of older stars. Faint, bluish spiral arms extend outward from the bulge, with a slightly disrupted appearance. These arms indicate the presence of ongoing, though perhaps subdued, star formation. The overall color profile suggests a galaxy undergoing a transition from a more active star-forming phase to a more quiescent state. There is some indication of tidal disruption as some of the arms are much fainter than others. 
