The galaxy presents as a centrally concentrated object with a diffuse, disturbed morphology. A significant portion of the galaxy's light appears to originate from a bright, unresolved core, possibly indicative of an active galactic nucleus or a dense stellar bulge. The overall shape deviates noticeably from a perfect ellipse, showing signs of irregularity. There is some disk-like feature, but it appears warped or disrupted. Faint, asymmetric extensions are visible, hinting at tidal interactions or ongoing merger activity. Patches of bluer light are observed in the surrounding regions of the galaxy, suggesting active star formation in the outer disk. The redder light in the center may be from older stellar populations. The light from the galaxy is generally compact, implying this galaxy is likely of intermediate size.
