The galaxy presents as a luminous, flattened elliptical form. Its central region exhibits a concentrated glow, suggestive of a substantial stellar population and potential presence of an active galactic nucleus, although further spectral analysis would be required to confirm this. The overall color profile appears somewhat reddish/yellowish, which could imply an older stellar population with a lower rate of ongoing star formation. The morphology appears generally smooth, lacking any clear spiral arm structures or significant dust lanes. The galaxy's shape is elongated, indicating a deviation from a perfect spherical form. There is no obvious visual evidence of any major mergers or tidal disturbances, although subtle signs of minor interactions could be present. The overall structure seems relatively undisturbed, implying a degree of dynamical stability.
