The galaxy presents a clear disk structure, viewed at an oblique angle, suggesting it may be a spiral or lenticular type. A prominent central bulge is visible, exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. Fainter, bluish regions extend outwards from the central bulge, concentrated particularly at the top and bottom edges of the disk. These regions may contain younger, hotter stars engaged in active star formation. There is some irregularity to the light distribution within the disk, which hints at possible disturbances. A faint, extended halo may be present surrounding the main galactic structure. Possible merging activity or tidal features cannot be ruled out based on morphological analysis.
