The galaxy presents as a single, centrally concentrated object with a smooth, diffuse light distribution. There are no prominent spiral arms, bars, or other distinct features readily apparent in the disk. The galaxy appears largely elliptical in shape, exhibiting a high degree of radial symmetry. The color profile shows a reddish hue in the core region, gradually transitioning to a bluer tint toward the outer edges. There is no clear evidence of ongoing major mergers or significant tidal disturbances, although subtle asymmetry and minor disturbances cannot be ruled out due to the image resolution. The galaxy’s light is dominated by older stellar populations, with a comparatively lower fraction of young, massive stars, suggesting a relatively low current star formation rate.
