The galaxy presents as a somewhat elongated structure. It is likely an early-type galaxy, exhibiting a dominant, smooth bulge with a high degree of central concentration. The central region shows a bright, yellowish hue, indicative of an older stellar population. Moving outward from the center, the light gradually fades, suggesting a decrease in stellar density. There is a subtle hint of a disk component, though it is not sharply defined, which contributes to its overall elongated shape. The outer regions exhibit a more diffuse, grayish color. There appears to be some minor irregularities in the outer structure, hinting at the possibility of past minor interactions or disturbances. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers or strong tidal interactions with nearby galaxies.
