The galaxy presents a concentrated morphology. A bright, dominant central bulge is clearly visible, exhibiting a notable intensity. The surrounding disk appears faint, with a slightly irregular form. There is possible evidence of a minor disturbance or interaction, suggested by a slight asymmetry in the disk structure; it seems that on one side, the material is more extended than the other. There is no strong indication of prominent spiral arms or a bar structure. Overall, the light distribution shows a gradient from blue in the core to more red colors in its outer components. The overall smooth appearance may denote this system to be an elliptical galaxy or potentially a spiral galaxy with a dominant bulge component observed at a moderate inclination. 
