The galaxy exhibits a generally irregular morphology, with no clear spiral arms or elliptical structure immediately apparent. A central bulge region is identifiable by its bright, concentrated luminosity. The disk, if present, appears somewhat disturbed or irregular in shape, with an estimated radius of approximately 2 arcseconds. There are hints of potential tidal features, but it is difficult to say for certain, and it could be an artifact. The central luminosity is bright, which may indicate a fairly bright region. It has a blue-ish tint, which means it is likely undergoing star formation, and there is a disturbance in the edge of the galaxy, which may indicate it is merging with a smaller galaxy.
