The galaxy presents with a somewhat irregular morphology, appearing elongated with a brighter, more concentrated central region that likely houses the galactic nucleus. Fainter, diffuse emission extends outwards from the center, suggesting the presence of a stellar disk or halo. The overall color of the galaxy is relatively blue, indicating a possible population of young, hot stars and ongoing star formation activity. Patches of redder hues, possibly due to older stellar populations or dust obscuration, appear to be present, especially within the central region. There is faint evidence of some disturbance or possible asymmetry, with the upper region perhaps being slightly more extended or diffuse compared to the lower region, which may point to a past minor merger event or tidal interaction.
