The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile with minimal discernible features. The central region shows a bright, yellowish-white core which gradually fades into a fainter, more diffuse halo. The overall shape appears to be approximately in between round and elliptical. There are no obvious spiral arms, dust lanes, or other features associated with spiral or irregular galaxies visible in this image. The color gradient suggests a population of older stars dominating the light emission, consistent with a low current star formation rate. There is no evidence of any major tidal disturbances or ongoing mergers.
