The galaxy presents as a centrally concentrated object with a generally smooth morphology, appearing elliptical in shape. The core exhibits a yellow-orange hue, suggesting an older stellar population likely dominated by red giant stars and a lack of ongoing significant star formation. Fainter, diffuse extensions surround the central region, showing a subtle gradient in color towards the outer edges. These extensions transition towards slightly redder tones compared to the core, possibly indicating a change in stellar population or dust content. There is no readily apparent presence of spiral arm structure, nor significant irregular features indicative of a recent major merger event. The overall appearance suggests a galaxy with a large stellar mass. There may be some very minor disturbances to the structure.
