The galaxy presents as a somewhat elongated, lenticular-shaped structure. Its overall color appears to be slightly reddish, implying an older stellar population and potentially lower rates of current star formation. The central bulge appears relatively smooth and dominant, with a gradual fading of luminosity towards the edges. There's little evidence of distinct spiral arm structures or prominent dust lanes. Faint extensions or tidal features are absent in this image, suggesting a lack of recent major merger events. The galaxy appears to be a relatively isolated system, undisturbed by strong gravitational interactions with neighboring galaxies.
