The galaxy presents a generally smooth, rounded morphology. The central region exhibits a concentrated luminosity, appearing bright and slightly yellowish, suggesting an older stellar population. A faint, diffuse halo surrounds the core, with a subtle bluish tint discernible at the periphery, possibly indicating the presence of younger stars or ongoing star formation, though this activity appears to be at a relatively low level. There is no indication of distinct spiral arms or a bar structure. No major merger events appear to be actively distorting the galaxy's shape. Overall, the galaxy appears to be an elliptical or lenticular galaxy, showing a more or less homogenous and evolved appearance.
