The galaxy presents as a relatively smooth, centrally concentrated object, appearing nearly circular in shape. There is little evidence of spiral arms or a prominent disk structure. The light profile suggests a bulge-dominated system, with a bright, yellowish core that gradually fades into a fainter, more diffuse halo. The color gradients indicate that the central region is redder compared to the outer regions, suggesting an older stellar population in the core. Any disk is very faint. There appears to be no significant ongoing star formation in this galaxy, consistent with its overall red color and smooth morphology. There is no indication of any major disturbances or ongoing merger activity.
