The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge that appears nearly spheroidal. The light distribution suggests a relatively smooth morphology, although subtle variations in color and intensity are visible in the outer regions. These may indicate the presence of faint, diffuse structures like stellar streams or tidal features. There is a possible hint of a disk component. The galaxy does not exhibit any obvious signs of ongoing or recent major mergers, but there may be a minor interaction or disturbance. The color indices suggest a stellar population that is moderately evolved, and the absence of strong blue colors suggests a lack of significant active star formation.
