This galaxy exhibits a roughly elliptical morphology, with evidence of a disk-like structure. It is tilted relative to our line of sight. A concentrated central bulge dominates the galaxy's core. The galaxy appears to have spiral arm features. These arms are somewhat flocculent and not tightly wound. The color distribution suggests the presence of both older stellar populations, indicated by the reddish hues, and younger, bluer stars, particularly concentrated in the arms and possibly some star forming regions. A weak bar feature seems to run through the galaxy's center. The overall structure indicates a system that is neither a pure elliptical nor a well-defined spiral, showing characteristics of both. The galaxy's light profile suggests that it could be actively forming stars, although at a moderate rate. There are no obvious signs of major mergers or significant tidal disturbances. The appearance is generally consistent with a spiral galaxy undergoing a period of relatively quiescent star formation.
