The galaxy presents as a cigar-shaped, smooth structure. There is a notable absence of prominent spiral arms or defined disk features. The light distribution suggests a concentration of stellar mass towards the center, with a gradual fading towards the edges, indicative of a spheroidal morphology. A smooth, diffuse halo surrounds the central region. No significant tidal tails, plumes, or distortions are observed, suggesting the absence of recent major merger events. The overall color appears relatively homogenous, with a slight gradient towards bluer hues in the outermost regions.
