The galaxy presents an overall elliptical morphology with a discernible central bulge. The disk component appears to be inclined relative to our line of sight. Spiral arm structures are not immediately apparent in this image, although some irregularity in the disk's light distribution suggests the presence of underlying features. Color gradients are observed, with the central bulge exhibiting a generally redder hue, potentially indicating a population of older stars. The outer disk appears bluer in comparison, which could suggest ongoing star formation regions or a younger stellar population. The galaxy lacks a prominent bar structure, although some asymmetry is noted near the core. There is no clear indication of a recent major merger event.
