The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. There is a general lack of discernible spiral arm structure or prominent dust lanes. The dominant color is yellowish-orange, suggesting an older stellar population and a relatively low rate of ongoing star formation. The overall shape is moderately round, with only a slight deviation from a perfect circular profile. There are no visible signs of major mergers or significant tidal disturbances. The color gradient suggests that the core is likely more luminous with light coming from an older stellar population with a lower concentration of dust compared to the outer regions. An object to the left appears blue which indicates the presence of younger stars.
