The galaxy presents as a moderately luminous, elongated spheroid. It exhibits a smooth, diffuse light distribution, suggesting a relatively uniform stellar population. The galaxy's color profile is dominated by redder hues concentrated toward the central bulge, transitioning to bluer tones in the outer regions. This suggests a possible age gradient, with older, redder stars in the core and younger, bluer stars in the disk. The high ellipticity indicates that this galaxy is likely an elliptical galaxy seen edge-on, or a spiral galaxy with a very tightly wound spiral arm structure and prominent bulge, also observed nearly edge-on. There is no immediately apparent evidence of active galactic nuclei, strong star-forming regions or significant dust lanes. There is no evidence of recent or ongoing major merger activity, but potentially minor distortions could be present.
