The galaxy presents a largely smooth and concentrated morphology. It is moderately elliptical in shape, not perfectly round, but without significant elongation. A bright central bulge is evident, exhibiting a high degree of luminosity. The galaxy color is a bluish white, suggesting a moderate population of younger, hotter stars, although the lack of distinct spiral arm structure suggests a predominantly older stellar population. There is no visually obvious presence of a strong disk component or prominent spiral arms. Minimal evidence of tidal features or major disturbances indicates no recent major merger activity, although minor asymmetrical features could be present at a low level. Overall, the galaxy appears to be an intermediate-mass system displaying characteristics of a smooth, relatively quiescent galaxy.