The galaxy presents a generally smooth morphology, with little evidence of distinct spiral arms or other prominent features. It appears elliptical, elongated in shape with an axial ratio suggesting it is seen at an angle. The galaxy exhibits a color gradient, transitioning from a brighter, yellow-orange core region to a fainter, bluer periphery. This color variation hints at a change in stellar populations across the galaxy, with older, redder stars dominating the central bulge, and a population of younger, bluer stars residing in the outer regions. No major disturbances or signs of recent merger activity are immediately apparent, though subtle irregularities may exist within the galaxy's diffuse outer halo.
