The galaxy presents as a relatively smooth, elliptical morphology. Its shape appears to be more in-between elliptical and round, showing some degree of flattening. The central region exhibits a strong concentration of light, indicative of a prominent bulge. There are no obvious spiral arms or bar structures visible. The color gradient suggests an older stellar population, trending towards redder hues in the inner regions with subtle blue-ish color in the more diffuse, outer regions. No significant dust lanes or prominent star-forming regions are apparent. The general form suggests the object has not experienced a recent major merger, though there may be very minor disturbances in the outer regions. Overall, this is a typical elliptical galaxy with a well-defined bulge and smooth light distribution.
