The galaxy presents an elliptical morphology, with a smooth light distribution indicating a lack of prominent spiral arms or significant disk-like structure. The core region exhibits a high surface brightness, characterized by a yellowish-orange hue, suggestive of an older stellar population. There is minimal indication of on-going star formation within the central region. The light intensity gradually decreases outward from the core, transitioning to a fainter, more diffuse halo. A subtle blue tint is observable within the outer reaches of the galactic halo, possibly indicative of a younger stellar population than what is seen centrally, or lower metallicity. There is no indication of significant tidal disturbances or ongoing mergers affecting the galaxy's structure. The object appears to be relatively isolated and undisturbed.
