The galaxy presents as a largely featureless, elliptical-like structure. There is a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Moving outwards from the core, the galaxy fades into a less distinct, more diffuse halo. The overall color shifts slightly towards a bluer tone in the outer regions, potentially indicating the presence of a younger, hotter star population, or ongoing star formation at a modest rate. The galaxy appears relatively smooth, lacking prominent spiral arms or strong dust lanes. A subtle asymmetry is visible. There is no indication of major mergers or significant tidal disturbances; it appears to be a fairly relaxed system. Its approximate physical size is roughly 8.6 kpc across, given the inferred distance based on redshift data.
