The galaxy presents as a moderately sized, relatively smooth object. It appears elliptical in shape, though it's not perfectly circular. A bright, concentrated central bulge is clearly visible, with a diffuse halo extending outwards. There's a slight flattening, suggesting the possibility of a disk component viewed at an angle that is somewhere near face-on. There does not appear to be defined structure, spiral arms, or prominent dust lanes. The color distribution shows a smooth gradient from a slightly bluer hue in the outer regions to a redder hue near the core. Given the apparent shape, smooth texture, and color distribution, it is likely a late-type spiral galaxy. The general morphology suggests that the system may be relatively evolved, though confirmation with higher-resolution imagery and spectroscopic data would be necessary for confirmation. There is no evidence of ongoing mergers or significant tidal interactions.