This galaxy appears to be of intermediate size and exhibits a somewhat amorphous morphology. The central region displays a smooth, diffuse light distribution, suggesting a relatively old stellar population or a lack of significant recent star formation. Moving outward from the center, there is subtle evidence of structural features. The overall structure is not perfectly smooth, but rather shows slight irregularities and a possible faint extension or tidal tail on one side, hinting at a past interaction or merger event. There is a marginal presence of blue light scattered throughout, this could possibly be from the presence of younger stars or active galactic nuclei. The color profile appears relatively uniform across the galaxy, with a tendency towards redder hues, consistent with an older stellar population dominating the overall light output.
