The galaxy presents as a relatively smooth, centralized light distribution. A slight ellipticity is observed, with a subtle extension along one axis, suggesting a possible deviation from a perfectly spherical shape. The core region is notably brighter and appears slightly more yellow or red-shifted. The outer regions appear fainter. No distinct spiral arm structures or prominent dust lanes are discernible. There is no evidence of major ongoing merger activity or significant tidal disturbances in the immediate vicinity of the galaxy. Color gradients suggest that the stellar populations may be somewhat older in the central bulge compared to the outer regions. The overall impression is that of a quiescent galaxy, possibly an elliptical or lenticular type, observed at a distance.