The galaxy presents an elongated, cigar-shaped morphology, appearing smooth with an absence of prominent spiral arm structures. A concentration of light towards the central region suggests a bulge component. The color distribution reveals a reddish core, potentially indicative of an older stellar population or dust obscuration. Progressing outwards from the core, a transition to slightly bluer hues along the disk is observed, suggesting the presence of younger, hotter stars, potentially in regions of ongoing star formation. There might be a faint disk-like structure, but the resolution is limited to confirm. Minor morphological disturbances may be present, though no major merging events are evident. Overall, the galaxy appears as a relatively evolved system with signs of both older and younger stellar populations.
