The galaxy presents as a moderately faint, relatively compact object. Its morphology appears largely smooth and elliptical, though with some elongation. The overall color profile suggests a predominantly older stellar population, with a lack of significant blue emission indicative of recent, widespread star formation. There is no prominent disk structure visible, nor any obvious spiral arm features. A slight asymmetry may be present in the isophotes, potentially suggesting minor interaction or disturbance in the past, but it is not definitively a merging event. The galaxy appears fairly isolated in its immediate vicinity.
