The galaxy presents a largely smooth morphology, appearing as a flattened spheroid. Its color profile exhibits a central concentration of redder hues, suggesting an older stellar population or significant dust obscuration in the core region. Fainter, bluer colors extend outwards from the central region, possibly indicating regions of more recent or ongoing star formation, particularly at what could be considered the "edge" of the galaxy. Overall, the galaxy lacks distinct spiral arms or other prominent features, leaning towards an elliptical or lenticular classification. There may be a very subtle hint of distortion or asymmetry in the outer regions, however more information is needed. The galaxy appears to be somewhat large and massive.
