The galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated luminosity profile. The core region appears bright and slightly blue-tinged, suggesting the presence of a younger stellar population or active galactic nucleus activity, though the image resolution limits definitive assessment. The surrounding halo exhibits a more diffuse, redder hue, indicative of older stellar populations. There is a notable lack of defined spiral arm structure or prominent dust lanes. The overall morphology suggests a galaxy that is either an early-type spiral or an elliptical galaxy, with the smoothness leaning toward the latter. Faint disturbances may be present in the outer regions, but are ambiguous. The galaxy appears to be undergoing a period of relatively quiescent evolution.
