The galaxy presents a generally smooth, elliptical morphology, appearing as a flattened spheroid. The light distribution suggests a relatively homogenous stellar population, lacking distinct spiral arms or prominent dust lanes. The core region exhibits a brighter, concentrated luminosity, indicative of a higher stellar density and likely a supermassive black hole. The overall color gradient transitions from a yellowish-white core to a redder outer halo, potentially revealing a shift in stellar composition. There are faint disturbances visible on the left side of the image, possibly due to a minor interaction with another galaxy. This interaction does not dramatically disrupt the smooth morphology of the galaxy. The object appears elongated, with the major axis significantly longer than the minor axis, suggesting an oblate spheroidal shape.
