The galaxy presents a generally smooth appearance, with a notable lack of distinct spiral arms or a prominent central bulge. Its morphology appears to be somewhere between round and elliptical. There's evidence of a possible merging event or tidal interaction, with some visible disturbance in the overall structure. The galaxy has a significant luminosity across the observed optical bands, suggesting a substantial stellar population. Star formation appears to be suppressed, indicating the galaxy is either a quiescent system or experiencing a lull in star-forming activity. The color distribution suggests an aging stellar population within the galaxy. A faint, diffuse halo or envelope of material may surround the main galactic body.
