The galaxy presents as a centrally concentrated object with a smooth, symmetrical morphology. It appears roughly elliptical in shape, exhibiting a gradual decline in luminosity from the bright core outwards. The central region is characterized by a yellow-orange hue, suggesting an older stellar population. There is little evidence of distinct spiral arms or prominent dust lanes. The overall color and lack of resolved features suggest that the galaxy is likely a relatively quiescent system. The absence of significant distortions suggests that it is not currently undergoing a major merging event, though subtle disturbances may be present.
