This galaxy appears to be a spiral galaxy, viewed at an oblique angle. It presents a flattened, disk-like structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting a population of older, redder stars. Fainter spiral arms extend outwards from the central bulge, tinged with hints of blue, potentially indicating regions of more recent star formation. The dust lanes appear subtle, mostly visible as slightly darker regions within the spiral arms and along the galaxy's disk. There are no strong indicators of ongoing major mergers or tidal disturbances, although a minor irregularity is present. Overall, the galaxy appears relatively well-defined and not highly disrupted.
