The galaxy appears to be an elliptical type, exhibiting a smooth and rounded morphology. Its light profile suggests a high degree of central concentration. There is a notable lack of distinct features such as spiral arms or dust lanes. The galaxy presents a yellowish-red hue, indicative of an older stellar population, potentially dominated by red giant stars. This spectral characteristic, coupled with the smooth morphology, suggests a relatively low rate of ongoing star formation within the galaxy. An additional object to the left of the main galaxy may be another galaxy that is undergoing a minor disturbance. There is no visible evidence of major interactions or mergers affecting the overall structure of the galaxy.
