The galaxy appears as a lenticular or possibly a spiral galaxy viewed edge-on. A central bulge is clearly visible, exhibiting a yellowish-orange hue, indicating a population of older stars and a relatively low rate of star formation. A faint, elongated disk extends outward from the bulge, displaying a bluer color gradient towards its outer regions, which suggests the presence of younger stars and ongoing star formation, but at a very low rate. There is no distinct dust lane visible along the equatorial plane. The overall morphology indicates a system that is predominantly smooth, with only minor disturbances if any. The apparent size of the galaxy is relatively compact, with its dimensions suggesting a moderate-sized galactic structure. The absence of any prominent tidal features or nearby companion galaxies suggests that it is likely not undergoing major interactions or mergers.
