The galaxy presents as a relatively compact system. A prominent, diffuse central bulge is visible, exhibiting a yellowish-white hue indicative of an older stellar population. Fainter, elongated features extend outward from the central region, possibly representing faint spiral arms or a disk component, although their morphology is poorly defined given the image resolution. These outer regions show bluer tinges, hinting at the presence of younger, hotter stars but minimal star formation. There are no clear signs of significant dust lanes or prominent HII regions. The galaxy exhibits a moderate redshift. Based on the morphology and colours, it would likely be a large, smooth galaxy. There may be evidence of some type of minor disturbance to the overall form of the galaxy, indicating a possible previous merger event.
