The galaxy presents as a luminous, elliptical object with a smooth, featureless morphology. The light distribution appears concentrated towards the center, indicating a dense galactic nucleus. The overall color profile tends towards the red end of the spectrum, suggesting a relatively older stellar population dominating its composition, with a lack of significant recent star formation activity. The galaxy appears elongated, with a cigar-like shape, implying a deviation from a perfect spherical symmetry. There is no evidence of major ongoing merger events or significant tidal disturbances affecting the galaxy's structure, although there may be some minor structural asymmetry.
