The galaxy presents as an elliptical or lenticular system, exhibiting a largely smooth and centralized light distribution. A prominent, bright central bulge dominates the structure, suggesting a high concentration of stars. The overall color appears yellowish-white, indicative of an older stellar population with fewer young, massive stars. There is little evidence of spiral arms or prominent dust lanes, supporting the classification of a relatively quiescent galaxy. The edges of the galaxy appear somewhat blurred and indistinct, which may be due to the limits of the image resolution. No significant morphological disturbances or tidal features are apparent, which suggests that there is no ongoing major merger activity or tidal interactions. 
