The galaxy presents a generally elliptical morphology, appearing mostly smooth with no readily discernible spiral arms or strong features. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. A gradual decrease in brightness is observed moving outward from the core toward the edge, though there appears to be a somewhat sharp drop in brightness around the nucleus. A slight elongation is apparent, deviating from a perfectly circular shape. There is a very slight blue hue to the galaxy, which could indicate the presence of younger stellar populations, however the yellow hue is dominant, suggesting an older stellar population. There are some faint hints of possible minor disturbances in the morphology, but these are not distinctly pronounced. Overall, the galaxy appears to be a relatively undisturbed system with a dominant elliptical shape.
