The galaxy presents as a moderately luminous, elongated, and relatively smooth object. Its light is dominated by a blue-white hue, suggesting the presence of a moderate population of relatively young, hot stars. The central region exhibits the highest luminosity, fading gradually outwards toward the galaxy's periphery. The overall smooth morphology indicates a lack of significant spiral arm structure or major disturbances. The galaxy appears to be an elliptical type galaxy that is slightly cigar-shaped with no obvious merger activity.
