The galaxy presents an overall elliptical morphology, with a noticeable elongation. A bright, relatively compact central region, possibly a bulge or active galactic nucleus, dominates the galaxy's luminosity profile. Emanating from this central region are faint, diffuse extensions exhibiting a blueish hue. These structures could potentially be tidal tails, stellar streams, or disrupted spiral arms. There is a slight indication of possible merging activity, as the shape appears somewhat irregular and the distribution of light within the extensions seems uneven. Overall, the system shows a complex morphology suggesting potential interactions or disturbances in its past. The observed colors suggest recent or ongoing star formation.
