The galaxy presents a somewhat elongated, lenticular appearance, with a relatively smooth morphology suggesting characteristics of an early-type spiral or potentially an elliptical galaxy. The central region exhibits a high degree of luminosity, indicating a concentrated stellar population or active galactic nucleus activity. Diffuse light extends outwards from the core, with a noticeable flattening of the disk. Some very faint and subtle features are visible, potentially signifying spiral arm remnants or tidal disturbances, but are not distinctly defined. The overall color profile appears moderately red, implying a population of older, cooler stars with limited ongoing star formation. No pronounced dust lanes or distinct star-forming regions are apparent within the galaxy. The galaxy appears relatively isolated, showing no immediate signs of major interaction with other galaxies.
