The galaxy presents an overall elliptical morphology, appearing largely smooth and centrally concentrated. Its color gradient transitions from a redder core to a bluer, more diffuse outer region. The core appears to be a dense concentration of older stellar populations, while the outer halo may be comprised of younger stars or the result of tidal interactions. There is a faint hint of distortion, possibly due to a minor interaction, which is suggestive of a non-relaxed system. Overall, the galaxy is characterized by a relatively low star formation rate. The galaxy is of intermediate mass and luminosity.
