This galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular classification. The galaxy presents with a bright, concentrated central region, and the light profile appears relatively diffuse outwards, lacking distinct spiral arm structures. There is a slight elongation, trending towards a rounded, but not perfectly spherical, shape. The color profile indicates a predominantly older stellar population, evidenced by the redder hues observed. There is no apparent major merging activity or significant tidal disturbance, although a minor irregularity cannot be ruled out based on the image resolution. Star formation appears to be occurring at a low rate.
