The galaxy appears as a centrally concentrated object, exhibiting a relatively smooth morphology. It has an elliptical shape, appearing elongated, but not extremely so. The core displays a bright, concentrated luminosity, suggesting a high density of stars in the central region. Progressing outwards from the center, there is a gradual decrease in surface brightness. Faint, diffuse light extends outwards from the central bulge, forming a more extended halo or disk-like structure. The overall color of the galaxy shifts subtly, from a yellowish hue in the core to a bluer tint in the outer regions. There are no clear indications of spiral arms, significant dust lanes, or other prominent features typically associated with late-type galaxies. The lack of strong morphological disturbances suggests that the galaxy is relatively undisturbed and stable. There is a very slight indication of minor irregularity in the halo, which may be evidence of minor merger or tidal interactions, but the smooth overall appearance dominates.
