The galaxy presents as a moderately bright, lenticular or early-type spiral system. Its core exhibits a concentrated, luminous glow, indicative of a substantial stellar population. The central bulge appears relatively smooth, lacking significant dust lanes or distinct morphological features.

Extending outward from the core, a faint, diffuse disk is observed. It appears relatively flattened, with a subtle color gradient suggesting a distribution of stellar populations, possibly with a small fraction of younger, bluer stars. Hints of spiral arms or other disk structures are subtle or absent.

The overall color profile suggests a relatively mature stellar population, with a redder hue dominant. Star formation activity appears to be moderate or low. There is no apparent interaction with nearby galaxies or distortions to its shape, suggesting that the galaxy is relatively isolated and dynamically stable. The approximate size of the galaxy appears normal for its type.
