The galaxy presents as a centrally concentrated object, exhibiting a predominantly smooth morphology. The central region appears luminous and yellow-white in color, suggesting an older stellar population. A slight extension of the light distribution can be seen towards the periphery of the galaxy, creating a diffuse halo-like structure. There appears to be a subtle asymmetry in the outer regions, potentially indicative of minor gravitational interaction or internal disturbances. The overall shape appears elliptical, with a slight deviation from perfect roundness. There isn't a notable presence of distinct spiral arms or prominent dust lanes. The color gradient suggests a relatively quiescent star formation rate.
