The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, potentially indicative of an older stellar population. There are no distinct spiral arm structures visible. Faint, diffuse extensions, predominantly showing blue and green tints, emanate from the core, suggesting the presence of some ongoing star formation. The galaxy does not show signs of major disturbances or interactions, though minor irregularities are present. The overall shape is generally rounded, with a slight deviation towards a more elongated form. 
