The galaxy presents as an elliptical morphology, with a smooth light distribution concentrated towards the center. A central bulge is visible and appears to be the brightest region. The galaxy exhibits a faint, extended halo surrounding the main body. The color of the galaxy shifts from a warm yellow hue in the core to bluer tones in the outer regions. Indications are present of a disk-like structure. Possible disturbances and faint extensions are present in the outermost regions of the galaxy, suggesting a recent or ongoing interaction with another galaxy. Star formation is likely occurring, predominantly in the outer regions and disk. The central bulge consists of older stellar populations.