This galaxy presents as a relatively smooth elliptical morphology. The central region exhibits high luminosity, with a color profile skewed towards bluer wavelengths. This core is surrounded by a more diffuse, extended halo of relatively lower surface brightness, which trends redder in color. A slight elongation is observed, classifying it as either an E4 or E5 on the Hubble scale. There is a distinct lack of spiral arm structures or prominent dust lanes. No significant tidal features or signs of recent major mergers are apparent, though subtle asymmetries cannot be entirely ruled out. Based on the smooth morphology, the galaxy is likely composed of an older stellar population that ceased rapid star formation.
