The galaxy exhibits a generally smooth morphology, with a centrally concentrated bulge region that appears largely spheroidal. There is faint and very diffuse disk structure apparent. The color of the central region is somewhat redder compared to the outer regions, possibly indicating an older stellar population. No clear spiral arms or bar structures are visible. There is no evidence of any major mergers, although some minor disturbances may be present, but are not clearly visible in this image. Overall, the galaxy appears as an elliptical or S0 type galaxy at this resolution, lacking strong features of ongoing star formation.
