The galaxy presents as a centrally concentrated, luminous object with a fairly smooth morphology. The core region exhibits a yellowish-white hue, which gradually transitions to a greenish-blue in the outer regions. The galaxy appears to be somewhat elliptical in shape, but is fairly round. There is no strong evidence of spiral arm structures or significant dust lanes visible in this image. There also aren't indications of tidal tails or other major disturbances in the galaxy's structure, suggesting it is not currently undergoing a major merger. The relatively smooth appearance and color gradients imply a galaxy dominated by an older stellar population, with ongoing, but relatively low, star formation activity. 
