The galaxy appears as a centrally concentrated object, with a generally smooth profile. The overall shape is somewhere between round and elliptical. There is a slight elongation, but the deviation from perfect circularity is not extreme.

The core region exhibits a yellowish-orange hue, suggesting an older stellar population. The light distribution decreases gradually with radial distance, indicating a lack of distinct spiral arm structures or other prominent features. There is no evidence of a strong central bar or ring-like morphology.

The galaxy presents no obvious signs of ongoing mergers or tidal disturbances in this image. The light profile appears relatively undisturbed, suggesting that it is a relaxed system. However, a minor asymmetry cannot be completely excluded.

Based on the color indices, star formation activity within the galaxy is likely suppressed, with the dominant light coming from evolved stars. The galaxy may be a relatively massive system, judging by its overall brightness.
