This galaxy appears to be a lenticular or elliptical galaxy, exhibiting a smooth, diffuse morphology. It possesses an elongated, cigar-like shape. The galaxy's core is relatively bright and concentrated, appearing yellowish, suggesting an older stellar population with lower levels of on-going star formation. Fainter blue hues are seen on the edges of the galaxy, potentially indicating some younger stars within the disk, or recent interactions. There appears to be no prominent spiral arm structure or dust lanes visible. The overall appearance suggests the galaxy is relatively isolated, with no obvious signs of major merger events or tidal disturbances.
