The object appears to be a galaxy exhibiting a predominantly elliptical morphology. It is characterized by a smooth, centrally concentrated luminosity profile, lacking discernible spiral arms or a prominent disk structure. The light distribution is relatively even, with a gradual decrease in brightness from the core outwards. The galaxy presents a yellow-orange hue, potentially indicating an older stellar population with diminished recent star formation. There is no evidence of significant dust lanes or tidal features suggestive of recent merger activity. Overall, the galaxy appears as a relaxed system nearing the end of its evolution.
