The galaxy presents as a slightly elongated, centrally concentrated structure with a relatively smooth overall appearance. The core region appears to be the brightest, exhibiting a yellowish hue. This may be indicative of an older stellar population dominating the central regions, with a possible dearth of ongoing star formation in the core. The galaxy's outer regions gradually fade in intensity, and I do not perceive any distinct spiral arms or bar structures. The overall colour gradient suggests a radial change in stellar populations, moving from older, yellower stars in the centre to possibly younger, bluer stars in the outskirts, although this is not strongly apparent. There is a slight asymmetry in the outer isophotes, hinting at a possible interaction, but there is no visual distortion beyond a slight change in shape. There do not appear to be any significant dust lanes obscuring the light from the galactic centre. The galaxy appears to be relatively undisturbed.
