The galaxy presents as a somewhat disturbed spiral type system, though potentially with more amorphous structure. The central bulge is compact and luminous with a yellowish color, suggesting an older stellar population. Extending outward, the primary structure of the galaxy seems to form a slightly warped disk-like component. Evidence of spiral arms is present, albeit not well-defined or tightly wound. These arms exhibit a patchy distribution of blue hues indicating ongoing or recent star formation, though areas of high concentration are not clearly visible. There's a suggestion of tidal features or minor interactions visible extending to the right of the galaxy, perhaps indicating a past or ongoing interaction with a smaller companion, or simply tidal disruption from a previous merger. Overall, the galaxy appears to be undergoing a period of moderate star formation activity, with signs of past dynamic interactions that have influenced its current morphology.
