The galaxy presents as a relatively smooth, centralized mass of light. Its shape appears to be somewhere between round and oblong, with a slight elongation suggestive of a possible disk-like structure, though such features are not immediately prominent. The light distribution is mostly even, lacking significant clumping that might indicate active star formation regions. There's a subtle color gradient, with the central region perhaps appearing slightly redder than the outer edges, possibly suggesting an older stellar population in the core. Overall, the galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or recent mergers, although closer analysis is needed to rule out minor disturbances.
