The galaxy presents as a somewhat elongated, disk-like structure. It exhibits a central bulge that appears bright and concentrated, with a yellowish-white hue. This suggests a population of older stars. The disk component displays a bluer color, indicating ongoing star formation. The galaxy's edges seem somewhat diffuse and irregular, possibly due to interactions or tidal effects, though no clear signs of major merging activity are immediately apparent. The overall structure appears relatively smooth, lacking prominent spiral arms or strong dust lanes. Based on color gradients, the star formation appears to be concentrated in the disk region. The galaxy appears to be relatively isolated, with no other obvious signs of nearby major companion galaxies.
