The galaxy presents an elongated, somewhat cigar-shaped morphology. The central region exhibits a bright, concentrated luminosity, suggesting a significant concentration of stars, likely an older stellar population. Surrounding this central bulge, there is evidence of a fainter, extended disk. This disk appears to be oriented edge-on, limiting direct observation of any spiral structure that might be present. There are hints of bluer regions along the edges of this disk which could indicate younger star formation regions. The galaxy appears to be undergoing some kind of disturbance. Further investigation with higher resolution imaging and spectroscopic data would be beneficial to ascertain the nature of these features and confirm the presence of ongoing or recent star formation.
