The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. A slight disk-like feature may be present, but it is not a dominant characteristic. The shape of the galaxy appears generally round, exhibiting a slight deviation towards an intermediate form. There is no strong evidence of major mergers or significant tidal disturbances. The galaxy's color profile suggests a higher concentration of blue light in the central regions, indicating a potential presence of younger stars and ongoing star formation in this area. The outer regions appear redder, pointing to an older stellar population.
