The galaxy presents as a relatively smooth, elliptical structure, with a concentrated, bright central bulge. There are no obvious spiral arms or significant dust lanes visible. The core exhibits a yellow-orange hue, suggestive of an older stellar population. The outer regions appear fainter and display a slightly bluer color, possibly indicating a younger stellar population relative to the core, but the blue is minimal. The overall shape leans toward a flattened spheroid rather than a perfect circle; it is not cigar-shaped. There's no clear evidence of major merging activity or tidal disturbances in this image, though a possible faint asymmetry in the outer regions is detected. Based on its smooth appearance, the galaxy is likely a mature system. The low star formation rate aligns with its dominant older stellar population.
