The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable central bulge. The light is concentrated towards the center, indicating a higher density of stars in that region. The colour profile shifts from a yellowish hue near the core to a slightly redder tone in the outer regions, suggesting a possible variation in stellar populations or dust content. The shape is close to round, with a possible subtle elongation. There is no clear evidence of spiral arms or significant morphological disturbances. The galaxy appears relatively isolated, with no obvious signs of ongoing major mergers or tidal interactions.
