The galaxy appears to be a disk galaxy with a prominent central bulge. The bulge region is a bright, concentrated source of light, possibly indicating a high stellar density or the presence of an active galactic nucleus. The disk component is relatively smooth and featureless, with no obvious spiral arms. The overall morphology suggests a relatively undisturbed system, although there may be some minor disturbances. The galaxy has a moderate angular size, appearing neither particularly large nor small. The color profile appears somewhat redder in the central regions, shifting toward bluer hues in the outer disk, which might indicate ongoing star formation. The disk edge shows some minor irregularities, potentially hinting at tidal interactions or past minor mergers. Overall, the galaxy appears to be a relatively normal, well-defined disk galaxy.
