The galaxy presents as a relatively compact object, exhibiting a flattened, disk-like morphology when viewed edge-on. There's a notable central bulge region that appears somewhat bright and concentrated. The bulge seems to have a slight color gradient, transitioning from a more yellowish-white core outwards. Along the plane of the disk, there are indications of dust lanes or dark bands that obscure the light from the stars within the disk itself, especially where it intersects the bulge's outer regions. These dust lanes add complexity to the galaxy's structure. Faint extensions are observed emerging from the disc which suggests the possibility of minor tidal disturbance or an interaction with a smaller object in the galaxy's vicinity. Based on the color profile, the galaxy has signatures of both young stellar populations within the disk and older populations in the bulge. Overall, the galaxy has indications that it is a relatively stable and evolved spiral structure, but with minor potential signs of disturbance.
