The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge with a high degree of symmetry. The light profile appears diffuse and lacks distinct spiral arm structures or prominent dust lanes. The color gradient transitions from a yellowish-white in the galactic center to a blueish hue in the outer regions, suggesting a potential difference in stellar populations, with older stars dominating the core and a younger population present in the disk. There is no clear evidence of ongoing major mergers or tidal disturbances, although the outer edges of the galaxy have a slightly irregular shape.
