This galaxy presents a distinctly elongated, cigar-shaped morphology. The color distribution indicates an older stellar population, with a central concentration of redder hues suggesting a bulge composed of evolved stars. A subtle, extended disk-like structure is perceptible. There is a small presence of what appears to be younger stellar population or ionized gas along the edges. The galaxy appears relatively undisturbed, lacking obvious signs of ongoing major mergers or tidal interactions. Given the smooth appearance, this is likely an elliptical galaxy.
