The galaxy presents as a lenticular or edge-on spiral morphology. Its structure appears relatively smooth, with a high degree of concentration towards the central bulge. The galaxy is elongated, displaying an axial ratio that suggests a disk is viewed at a steep inclination. There is no prominent evidence of strong spiral arm structure in the image, though subtle color variations imply possible spiral density waves. The color profile indicates the presence of older stellar populations, with a gradient towards redder hues in the central region. There is a subtle blue tint visible throughout the galaxy suggesting a low level of on-going star formation. No significant tidal features or disturbances are evident, suggesting the galaxy is relatively isolated and not currently undergoing a major merger event. The overall impression is that of a relatively quiescent galaxy in a late stage of evolution.
