The galaxy presents a largely smooth morphology, exhibiting a high degree of circular symmetry. The light is concentrated in the center, and appears to fade outwards. The galaxy appears to be quite compact in extent, the size of which would be approximately 4 kpc. The galaxy exhibits an orange-red hue, suggesting a population of older stars, and diminished star formation. There is no evidence of significant spiral arm structures or active galactic nucleus. It appears to be a relatively quiescent system, with a notable absence of blue light indicative of young, hot stars. The high degree of smoothness suggests a minimal ongoing interaction with other galaxies.
