The galaxy presents as a slightly inclined spiral with a dominant central bulge. The bulge exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population. Faint spiral arms extend outwards from the bulge, displaying a patchy distribution of bluer light indicative of regions of ongoing star formation. Dust lanes may be present within the spiral arms but they are difficult to resolve at this resolution. The overall color of the galaxy leans towards the red end of the spectrum, particularly in the bulge region, suggesting a relatively low star formation rate. The galaxy appears to be undergoing a minor interaction or perhaps a merger event, indicated by a slight distortion in the spiral arm structure. There are minor disturbances that could mean there's a companion galaxy nearby affecting its shape. Its overall shape appears to be somewhere between round and cigar-shaped.
