The galaxy presents as a roughly elliptical, though somewhat irregular, form. The central region exhibits a high surface brightness, appearing nearly unresolved and intensely luminous. Moving outward from the center, the surface brightness diminishes, but color variations become apparent. The inner regions display a bluer hue, possibly indicating a population of younger, hotter stars. Fainter, redder components become more prominent in the outer reaches of the galaxy, suggesting an older stellar population. There is a slight asymmetry in the light distribution, with a subtle extension or tidal feature on one side. No spiral arm structures are clearly visible within the galaxy's extent. However, based on the subtle asymmetries the galaxy could be undergoing a minor merger.
