The galaxy presents a largely smooth morphology, with a dominant central bulge that appears somewhat rounded in shape. There is faint evidence of a disk-like structure extending from the central region, though any spiral arm features are not clearly distinguished in this image. The core appears to have an intense and relatively uniform light, suggesting a possibly older stellar population and/or significant dust obscuration. The color profile indicates a relatively red hue for the central region, transitioning to slightly bluer colors in the outer regions, indicating a potential population of younger stars and ongoing star formation in the outer regions. There is no clear visual evidence of strong tidal interactions or recent major mergers, however, minor disturbances cannot be ruled out based on the available image resolution. The galaxy seems to be of intermediate size, relative to the other observed galaxies.
