The galaxy presents a generally elliptical morphology, exhibiting a relatively smooth light distribution. The central region displays a high concentration of luminosity, suggesting a prominent galactic nucleus or bulge. Surrounding this central region, the galaxy extends into a more diffuse halo, with the outer edges gradually fading into the background. There appears to be evidence of tidal disturbance and/or an ongoing merger event, as indicated by asymmetrical features and potential distortions in the outer halo. The color profile suggests a higher concentration of older stellar populations, indicated by the redder hues, particularly within the core. There is a slight indication of bluer regions in the outer edges. The lack of distinctly resolved spiral arms or prominent dust lanes suggests that the galaxy is likely an elliptical or lenticular type system, possibly undergoing significant interactions.
