The galaxy appears as an elongated, disk-like structure with a noticeable central bulge. The bulge is the brightest region, exhibiting a yellowish-white hue, suggesting an older stellar population. Moving outward from the bulge, a fainter disk is observed. The disk presents a more diffuse and mottled texture, with hints of bluer regions interspersed. Overall, there is a relatively smooth appearance, with subtle features, but no obvious distinct spiral arm structures or strong dust lanes are discernible. The overall ellipticity of the galaxy is moderate, implying an inclination angle that is neither close to face-on nor edge-on. There are no major signs of tidal disruption or interactions with other galaxies, although there is a possible minor disturbance within the disk's structure.
