The galaxy presents as a moderately bright, elliptical object with a smooth, diffuse morphology. There is a distinct color gradient, transitioning from a more concentrated yellowish-white core to a fainter, slightly redder halo. The central region appears relatively uniform in texture, lacking any distinct spiral arm structures or prominent dust lanes. There is a small, faint, bluish object to the left of the galaxy, but further observation is needed to confirm if it is a part of the main system or a background object. Overall, the galaxy seems to be a mature system, possibly an elliptical galaxy, exhibiting characteristics of an older stellar population with low current star formation activity. There may be subtle signs of minor gravitational disturbances in the overall symmetry of the galaxy, suggesting a possible past interaction. Further spectroscopic analysis is required to determine its exact nature, redshift, and stellar population characteristics.
