The galaxy presents as a luminous, centrally concentrated system with a generally smooth morphology. Its form is largely elliptical, appearing mostly round on the plane of observation, with minimal discernible disk features. A gradual decline in luminosity is observed from the center outwards, with no prominent spiral arms or bar structures visible. The galaxy exhibits a yellow-white color indicative of an older stellar population. Areas of redder light are seen near the galaxy, possibly signifying regions of dust or ongoing, albeit low, star formation. A lack of strong blue emission suggests a relatively passive galaxy with diminished recent star-forming activity. While the main body appears undisturbed, there is a slight asymmetry on the edges, which indicates a possible tidal interaction.
