The galaxy presents as a slightly elongated, concentrated light source. The core is a bright, yellowish-white, suggesting an older stellar population is dominant within the central bulge. The color suggests a lack of ongoing, significant star formation in this region. Surrounding the core is a more diffuse halo with a faint disk. The overall structure appears relatively smooth, although subtle irregularities or faint arms may be present but are difficult to discern. The color of the surrounding disk appears slightly redder than the core, which could point to an aging stellar population. There is no obvious evidence of active galactic nuclei activity or any signs of a recent or ongoing major merger event, although some tidal features or minor disturbances cannot be ruled out at this resolution. The galaxy's overall morphology leans towards an early-type spiral, exhibiting characteristics of both elliptical and spiral galaxies, or possibly a lenticular galaxy.
