The galaxy presents as a disk-shaped system, likely a spiral galaxy viewed at a significant inclination. A central bulge is apparent, exhibiting a bright yellowish hue, possibly indicating an older stellar population. The disk shows a mottled texture, which could be due to the presence of dust lanes or variations in the density of star formation regions. 

The overall color profile of the disk ranges from yellow to red, implying a mix of stellar ages, with a potential gradient towards redder, older stars in the outer regions. There is little indication of active star formation, as indicated by the lack of bright blue regions typically associated with young, hot stars. The disk appears relatively smooth and undisturbed, without obvious signs of major mergers or significant tidal interactions. A slight distortion in the shape, giving it an elongated appearance, could suggest minor interactions or internal dynamical processes at play.
