The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded, with a concentrated central bulge that fades gradually into its outer regions. There is no clear evidence of spiral arm structure or a distinct disk component. Color gradients suggest an older stellar population, particularly within the bulge, exhibiting a yellowish hue, that fades to redder colors. This red-shift may also contribute to the reddish coloration. There appears to be no active merging or major disturbance. A faint, diffuse halo may be present, extending beyond the main body of the galaxy.