The galaxy presents as an elliptical morphology, elongated along its major axis with an estimated axis ratio of approximately 0.6. The light distribution exhibits a smooth profile, increasing in intensity towards a bright, concentrated nucleus. No distinct spiral arm structures or dust lanes are discernible in this image. The overall color appears redder in the central bulge region, gradually becoming bluer towards the outer regions. This color gradient may suggest a difference in stellar populations, with older, redder stars dominating the bulge and younger, bluer stars present in the galactic disc. Evidence suggests minimal disruption or interactions, indicating a relatively undisturbed evolutionary history.
