The galaxy presents an elongated, cigar-like morphology. Its central region exhibits a concentrated luminosity, appearing smooth and relatively featureless. The overall color profile suggests a mixture of stellar populations. The central bulge appears to be dominated by older, redder stars, giving it a yellowish-orange hue. Moving outward from the core, the galactic disk becomes faintly visible, displaying a bluish tint. The shape suggests it is an elliptical galaxy, possibly of type E4-E7, seen nearly edge-on. There is no sign of recent major merging activity or major disturbance in the galactic structure. However, subtle irregularities in the outer regions might indicate minor gravitational interactions or the remnants of previous, smaller merger events. Star formation appears to be ongoing, albeit at a moderate rate, concentrated within the disk region.
