The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a smooth, centrally concentrated light profile. It has a cigar-shaped appearance, suggesting a significant ellipticity. The galaxy is relatively compact, with a concentrated core and a fainter, more diffuse halo. There are no visible spiral arms or dust lanes. The galaxy's color suggests a population of older stars, with minimal evidence of recent star formation. There is no apparent tidal debris or other signs of a recent major merger event, though minor disturbances cannot be ruled out. Its alignment suggests it may be viewed close to edge-on. The overall morphology indicates a dynamically evolved system.
