The galaxy presents as an elongated, cigar-shaped object, strongly suggesting an elliptical morphology when viewed from our perspective. Its light profile appears relatively smooth, lacking prominent spiral arm structures or significant knots of star formation, which is further indicative of an elliptical galaxy. The core region exhibits a brighter, more concentrated luminosity, transitioning gradually to fainter outskirts. The galaxy presents a reddish hue, more concentrated towards the center. This color gradient could suggest an older stellar population, which is typical in elliptical galaxies, with younger bluer stars possibly present in small concentrations on the periphery. Its observed shape suggests a degree of flattening, but without higher resolution imaging, it's difficult to discern if this is due to intrinsic shape or viewing angle. It appears to be undisturbed.