The galaxy presents a generally smooth morphology with an elliptical shape, exhibiting a high degree of central concentration. There are no prominent spiral arms or a well-defined disk structure visible. The galaxy's light profile appears relatively uniform, with a gradual decrease in brightness from the core to the outer regions. There is a slight elongation observed, but the object is overall in between a round and cigar shape. There is no obvious evidence of any major mergers or significant tidal disturbances affecting its overall structure. Based on the color indices, the galaxy is more luminous in redder wavelengths than blue wavelengths. Overall, the color is on the redder side. This suggests an older stellar population is dominant, with lower levels of ongoing star formation.
