The galaxy presents a flattened, elliptical morphology, viewed at a significant inclination relative to our line of sight. A central bulge dominates the galaxy's structure, exhibiting a concentrated and relatively smooth distribution of light. Fainter, diffuse light extends outwards from the bulge, suggesting a disk component. Dust lanes are potentially present, based on subtle asymmetries within the disk, though the resolution is limited. There may be faint evidence of spiral arm structure, however this is not certain. The overall color profile suggests a mix of stellar populations, with the bulge likely composed of older, redder stars, while the disk may contain younger, bluer stars.
