The galaxy presents a generally smooth morphology, with a notable central bulge. It appears to be elliptical in shape, exhibiting a degree of elongation. There's a slight indication of a disk-like structure or perhaps faint spiral arms, but this is not distinct. The core region shows a concentrated luminosity, likely indicating an older stellar population. There's a lack of significant dust lanes or active star-forming regions, which reinforces the impression of a more evolved and quiescent system. The color gradient shifts from a slightly bluer hue in the outer regions to a redder tone toward the center, suggesting a spatial variation in stellar populations. Evidence for interactions with other galaxies appears minimal; there are no clear tidal tails or other morphological distortions indicative of recent merger events.
