The galaxy exhibits a roughly elliptical morphology, with a bright, concentrated central bulge that transitions into a more diffuse halo. The color profile indicates a yellow-white core, which may suggest an older stellar population dominating the bulge. Surrounding the core is a bluer region, suggesting more recent star formation compared to the core. Faint, disturbed features emanate outwards from the central region, that may be evidence of tidal interactions. The overall structure lacks a well-defined spiral arm structure, but the uneven distribution of the blue regions implies internal disturbances, potentially the result of a minor merger event. 
