The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears yellowish, suggestive of an older stellar population. The main body of the galaxy appears moderately round with only a slight deviation from perfect circularity. There may be a faint, diffuse disk or halo surrounding the bulge, but this is not clearly defined. There's no strong evidence of distinct spiral arms or prominent dust lanes. Overall, it appears to be a passively evolving system with little ongoing major star formation. The galaxy does not seem to be undergoing any major merger activity, or exhibiting large gravitational disturbances.
