The galaxy presents as a somewhat elliptical, centrally concentrated light source, indicative of an early-type system. The morphology appears largely smooth, with a high degree of symmetry. There's a slight elongation, but the overall shape is closer to round than cigar-shaped. There's no obvious presence of spiral arms or a prominent disk structure. 

Color gradients are present, transitioning from a bluer hue in the center to a redder hue in the outer regions. The bluer central color may suggest ongoing or recent star formation in the core, whereas the redder outer regions may be dominated by an older stellar population. No distinct tidal tails or strong evidence of recent major merger events are visible, though a subtle asymmetry on one side might indicate minor disturbance.
