The galaxy presents as an elliptical morphology, with a smooth light distribution. The central region exhibits a brighter, more concentrated luminosity, transitioning to a more diffuse halo. The galaxy appears slightly elongated, not perfectly spherical. There is no obvious spiral arm structure or dust lane features. The overall color appears yellowish, possibly indicative of an older stellar population. No significant signs of tidal disturbances or ongoing major mergers are observed; however, subtle irregularities in the outer halo cannot be entirely ruled out with this image resolution. There may be a small amount of star formation present.
