The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. A disk is either not present or is at an angle to be too difficult to observe. The galaxy exhibits a color gradient, transitioning from a yellow-white core to a slightly bluer outer region. This suggests a radial variation in stellar populations or dust content. The smooth appearance and color profile are consistent with a mature stellar population, though the slight bluing in the outer regions could indicate some ongoing, albeit low, levels of star formation. There is no visual evidence of significant tidal disturbances or ongoing major mergers, although a very subtle irregularity in the outer halo on one side could suggest a minor interaction event in the past. The galaxy appears to be well-defined and relatively isolated, and the light emitted appears relatively bright.
