The galaxy presents as a centrally concentrated, luminous object, exhibiting a smooth morphology indicative of an elliptical galaxy. The galaxy's overall shape approximates a flattened spheroid, with a slight elongation. The color profile suggests an older stellar population, dominated by redder wavelengths, particularly in the central bulge. There are no apparent spiral arms or significant dust lanes. The galaxy's smooth, featureless appearance suggests a relatively quiescent history, with minimal evidence of recent major mergers or active star formation. There is minimal distortion of the galaxy suggesting it is relatively isolated and not undergoing any major tidal disturbances or interactions with other galaxies. The central region appears to be a high luminosity, suggesting a potential active galactic nucleus. 
