The galaxy presents a generally smooth and rounded morphology. The light is concentrated towards the center with a bright, yellowish core, indicating a likely bulge component. There is a faint, diffuse disk surrounding the core, exhibiting a slight blue tint. This suggests some ongoing star formation activity, though likely not at a very high rate given the relatively subtle color. There appear to be some minor disturbances in the galaxy's structure, although it does not seem to be undergoing a major merger. It has a compact structure. The galaxy appears to be isolated. 
