The object appears to be a relatively compact galaxy. It exhibits a bright central region, which likely indicates a concentration of stars and possibly an active galactic nucleus. The light distribution appears somewhat irregular, with hints of non-uniform structures. There is no clear spiral arm structure or defined disk component visible, suggesting that it could be an elliptical or irregular galaxy, or a disk galaxy viewed at a high inclination. The colour distribution indicates a range of stellar populations, with bluish hues concentrated in some areas, possibly indicative of recent star formation. Redder regions may indicate older stellar populations or dust extinction. There may be indications of minor tidal disturbance, though there is no conclusive sign of major mergers or interactions with other galaxies.
