The galaxy appears to be a relatively smooth, elliptical-like structure with a centrally concentrated bulge. The core region exhibits a yellowish hue, suggesting a population of older stars. Moving outward from the core, the color transitions towards a bluer shade, possibly indicating the presence of younger stars in the outer regions. The galaxy appears fairly isolated with no obvious signs of major mergers or tidal disturbances. It seems to have a well-defined, round shape with a high degree of symmetry, showing no apparent strong spiral arm features or a prominent disk component. The overall morphology suggests a classification along the elliptical sequence, with a possibility of belonging to the S0 lenticular class. Star formation may still be occurring, but at a lower rate.
