The galaxy presents as a somewhat disturbed disk galaxy, with a noticeable bulge. The disk appears to be inclined relative to our line of sight. There are hints of spiral arm structure, though they are not well-defined, instead appearing somewhat flocculent and disrupted. A bright central region indicates the likely presence of an active galactic nucleus or a region of intense star formation. The galaxy exhibits a range of colors, with bluer regions suggesting ongoing star formation and the presence of younger, hotter stars, particularly within the disk. Redder regions may indicate older stellar populations. There is some indication of tidal features or interactions, potentially indicating a recent or ongoing merger event.
