The galaxy presents as a relatively compact, smooth object with a centrally concentrated luminosity profile. The overall color appears slightly blue-white, suggesting the presence of a moderate population of young, hot stars, though the smoothness indicates that any ongoing star formation is not dominating the overall light output. It is largely elliptical with a high degree of symmetry, lacking any obvious spiral arm structure or significant tidal disturbances. The shape is predominantly round, exhibiting only a subtle deviation toward a more elongated form. There is no evidence of an active galactic nucleus or intense starburst activity observable in the visual spectrum, nor any signs of ongoing major merger events. The outer regions fade gradually into the background sky, consistent with a high level of internal uniformity.
