The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggestive of a dense stellar population. The color profile transitions from a yellow-white center to a faint, diffuse blue halo, indicative of some ongoing, albeit minimal, star formation activity within the galaxy's outer regions. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy's overall shape appears close to round. There are no signs of tidal tails or other morphological disturbances characteristic of major merger events; however, there is a slight asymmetry in its outer reaches, possibly the result of a minor gravitational interaction.
