This galaxy presents as a moderately luminous, elliptical system, exhibiting a smooth, featureless morphology. Its overall shape appears somewhat elongated, transitioning from a bright, concentrated central region to a fainter, more diffuse outer halo. Color gradients are subtle, with the core displaying a yellowish hue suggestive of an older stellar population. There is no apparent spiral structure, dust lanes, or significant tidal distortions indicative of recent merger activity. Minor irregularities in the outer isophotes cannot be ruled out, but are not readily discernible. Based on its visual characteristics, the galaxy is likely to have undergone a significant portion of its star formation in the past, leading to a population of older, redder stars dominating its overall appearance.
