The galaxy presents as a single, largely amorphous structure. Its overall shape is elliptical or spheroidal, displaying a high degree of central concentration. The core region exhibits a warmer, yellowish hue suggestive of older stellar populations. Surrounding the core, the galaxy fades into a bluer, less defined region. This outer halo shows no discernable spiral arm structure or distinct features. The gradient between the core and the outer halo appears smooth, lacking sharp boundaries. There is no strong evidence of ongoing major mergers or tidal disturbances, though a slight asymmetry could indicate a minor interaction in its past. Overall, the galaxy appears to be a relatively relaxed system, likely populated by older stars and potentially exhibiting a low star formation rate.
