The galaxy presents an elliptical morphology, with a smooth and diffuse light distribution, suggesting an older stellar population. There is a slight elongation to the galaxy's shape, appearing somewhat cigar-shaped. The central region exhibits a higher concentration of light, appearing brighter than the outer regions, likely due to a higher density of stars in the galactic nucleus. Faint reddish hues are subtly visible within the central bulge, possibly indicating the presence of dust or a population of older, redder stars. There is no clear evidence of spiral arms or active star formation. Minor irregularities may exist but the image resolution is too low to discern these clearly. Overall, the galaxy appears relatively isolated and undisturbed, showing no signs of major mergers or tidal interactions.
