The galaxy presents as an elliptical morphology. It appears to be primarily smooth in texture, lacking any distinct spiral arm structures or significant dust lanes. The central bulge is concentrated and exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy gradually fade into the background sky, forming a diffuse halo. There is minimal evidence of ongoing star formation based on the color profile and absence of blue knots or HII regions. The galaxy is not exhibiting obvious signs of tidal interaction or morphological disturbance, indicating a relatively isolated state. The galaxy displays a moderate redshift, placing it at a considerable cosmological distance.
