The galaxy presents an elliptical morphology, elongated along its major axis. A bright, concentrated central bulge dominates the structure. Moving outward from the core, the luminosity decreases gradually, indicating a smooth transition to the outer regions of the galaxy. No distinct spiral arm features are discernible. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, possibly indicative of a higher concentration of evolved stars. There are hints of possible minor tidal disturbances or interactions, subtly affecting the overall morphology. The galaxy does not appear to be undergoing a major merger event.
