The galaxy presents as an elongated, elliptical structure. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. Moving outwards from the core, the luminosity gradually decreases into a fainter halo. The overall color profile appears somewhat redder. There is a slight curvature to the galaxy's form, indicating the potential for a warped disk or tidal interaction, although no clear signs of ongoing major mergers are readily apparent. Within the extent of the galaxy, there is not evidence of distinct spiral arm structures or prominent dust lanes.
