The galaxy presents a somewhat flattened, disk-like structure. The central region exhibits a bright, concentrated bulge which appears smooth in texture. This bulge is slightly elongated along the major axis of the disk. Extending outwards from the bulge, a faint disk is visible, showing some evidence of structure but appearing mostly smooth. The galaxy’s color profile suggests ongoing star formation, with bluer hues in the disk and a redder tint in the bulge. There is no prominent spiral arm structure readily apparent, though there is some indication of possible disturbances or tidal features along the edges, potentially hinting at past minor interactions. Overall, the galaxy appears to be a disk galaxy with a dominant bulge component, showing signs of possible recent or ongoing mild interaction.
