The galaxy presents a generally smooth morphology with an elliptical shape. A slight elongation is observed, although it largely appears rounded. The central region exhibits a concentrated, bright yellowish hue, indicative of an older stellar population likely dominated by evolved stars. The color profile suggests minimal ongoing star formation within the core.

The outer regions of the galaxy gradually fade, exhibiting a more diffuse, less defined structure. The color shifts to a slightly bluer tone in the outskirts compared to the core. There appears to be a subtle, low-intensity disk-like structure that cannot be ruled out. No prominent spiral arms or other distinct features such as dust lanes are visible. There is no evidence of any major disturbances in the surrounding vicinity.
