The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that is colored yellow, suggesting an older stellar population within the core, consistent with a lack of significant recent star formation. The galaxy is not perfectly spherical; it possesses a slightly elongated shape. There is no apparent presence of spiral arms or a well-defined disk structure. The lack of blue colors or distinct features like dust lanes further supports the conclusion of an older stellar population with little ongoing star formation. There are no signs of any major merger activity or significant tidal disturbances in the galaxy's morphology. The light profile suggests the galaxy is relatively compact.
