The galaxy presents as a well-defined, elongated structure with a pronounced central bulge. There is a color gradient across the galaxy, with a yellowish-white hue dominating the central regions, likely indicating an older stellar population. Progressing outwards from the center towards the edges, the color shifts towards a bluer tone which might indicate regions of more recent or ongoing star formation. The galaxy appears relatively smooth with no clear spiral arm structures visible; its morphology could be described as lenticular. The overall shape is reminiscent of a flattened spheroid. There is no evident dust lane or any major disturbances that disrupt the galaxy's shape, suggesting it has not undergone a major merger recently. The light distribution follows a concentrated central region. The outer regions are dimmer and the light is distributed sparsely.
