The galaxy presents as a relatively smooth, concentrated structure. It exhibits a predominantly elliptical morphology, with a high degree of roundness and a lack of discernible spiral arms or a prominent disk component. The central region displays a bright, concentrated core, suggesting the presence of an active galactic nucleus or a high density of stars. The color profile indicates a redder hue, likely due to an older stellar population and lower ongoing star formation activity. There is no evidence of significant tidal disturbances or interactions with other galaxies in its immediate vicinity. Overall, the galaxy appears to be a passively evolving system.
