The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. Its overall shape appears somewhat elongated, transitioning from a brighter core outwards. There is a hint of what appears to be disk-like structure, but the light is dominated by the bulge. The color profile is characterized by a yellowish to reddish hue, suggesting a population of older stars. Faint, diffuse extensions are present around the main body of the galaxy, possibly indicating a halo. There is no clear evidence of active star formation regions or distinct spiral arm structures. The galaxy does not exhibit obvious signs of major mergers or significant tidal disturbances.