The galaxy presents an overall smooth morphology, suggesting an elliptical classification or a spiral galaxy viewed at a high inclination. Its shape appears somewhat elongated, deviating slightly from a perfectly circular form. The central region exhibits a higher concentration of light, indicative of a galactic bulge. The color profile suggests a population of older stars, with a hint of blue light in the outer regions indicating some ongoing, albeit limited, star formation. No distinct spiral arms or prominent dust lanes are visible. There are no signs of major disturbances in the galaxy's structure, which suggests that it may not be actively merging with another galaxy.