The galaxy presents a generally elliptical morphology, with a dominant smooth component. There is some evidence of a fainter, more diffuse structure that may represent a disk, although it is not clearly defined. The central region is brighter, exhibiting a yellow hue, possibly indicative of an older stellar population. There is a slight asymmetry in the galaxy's overall form, potentially suggestive of a minor interaction or disturbance. The galaxy appears relatively isolated within its field.
