The observed galaxy presents as a somewhat elliptical structure with a smooth, centrally concentrated luminosity profile. It appears relatively featureless, lacking distinct spiral arms or prominent dust lanes. The color is generally consistent with an older stellar population, exhibiting a yellowish-red hue. The galaxy has a definite central bulge that fades outwards into a less luminous halo. The object's ellipticity suggests some degree of flattening in its overall shape. There is no visible evidence of ongoing major mergers or significant tidal disturbances within the observable structure. The object's smoothness gives it a round like shape. The absence of bright blue regions indicates a low rate of recent or current star formation activity.
