The galaxy presents as a luminous, elliptical object, exhibiting a relatively smooth morphology. It shows a concentrated central bulge with a gradual falloff in luminosity towards its outer regions. The color profile suggests an older stellar population, appearing generally yellow-red. The galaxy appears fairly isolated, with no obvious signs of ongoing major mergers or strong tidal interactions. There may be slight irregularities in the outer regions suggesting minor past interactions, although they are not strongly pronounced. The overall structure is indicative of an evolved system, consistent with an elliptical classification.
