The galaxy presents an overall elliptical morphology, appearing relatively compact. The central region is characterized by high surface brightness, exhibiting a bright, concentrated core. Moving outward, the intensity of light gradually diminishes, transitioning into a diffuse halo structure. 

A faint, extended feature or tidal tail is visible in the galaxy's vicinity, suggesting possible gravitational interactions. It's plausible that the main galaxy is undergoing a minor merging event. 

The color profile indicates a predominantly older stellar population, with a yellowish-red hue dominating the galaxy's light. Fainter, blueish regions can be distinguished which suggest areas of on-going or recent star formation. 
