The galaxy presents as a single, largely featureless object with a concentrated central bulge. Its overall morphology appears smooth, lacking well-defined spiral arms or a distinct disk structure. The light profile is centrally peaked, with a gradual falloff in intensity towards the outer regions. The object's shape can be described as elliptical or near-spherical, with only a slight elongation. The galaxy exhibits a yellowish-white hue, suggesting an older stellar population with a low rate of active star formation. There is no visual evidence of ongoing merger activity or tidal disturbances.
