The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated central bulge is apparent, exhibiting a yellowish hue, indicative of an older stellar population. The galaxy fades gradually from the bright core into the surrounding space. A faint disk structure might be present but isn't particularly prominent. No major signs of ongoing mergers or significant tidal disturbances are discernible. The galaxy appears to be fairly isolated and well-defined. The overall light distribution is concentrated, with only a minimal extended halo observed. There is a possible very slight flattening, but it is nearly round.
