The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The galaxy appears relatively smooth, with minimal evidence of spiral arms or distinct features. The overall shape is somewhat elongated, but largely homogenous. Faint, diffuse light extends outwards from the central region, diminishing in intensity with increasing radial distance. There is some indication of a slight flattening towards the outer edges, trending toward a more disk-like morphology, but it is dominated by the spherical symmetry. There is a mild amount of redder material within the core of the galaxy, whereas the outer region is bluer in color. There are no visible signs of significant recent merger events.
