The galaxy presents as a relatively smooth, elliptical-like structure. There is a distinct, concentrated central bulge that appears quite bright. The overall light distribution is concentrated toward the center. While the image quality is limiting, there are no apparent spiral arms or significant dust lanes visible. There is a faint halo of light surrounding the central region. The galaxy appears to have a fairly regular morphology, and there is no obvious evidence of recent or ongoing major mergers or tidal disturbances. The object seems to be a well-formed galaxy dominated by an older stellar population.
