The galaxy presents as a singular, largely homogenous object with a notable central concentration of luminosity. Its overall form approximates a rounded shape, exhibiting a gradual decrease in surface brightness extending from the core region outwards. No distinct spiral arms or bar structures are discernible, suggesting it may be a lenticular or elliptical type galaxy. There are no signs of ongoing mergers or major tidal disturbances. The color profile exhibits a yellow to slightly reddish hue, which would indicate an older stellar population and low star formation. The galaxy presents as a relatively smooth object, with only faint indication of a possible disk.
