The galaxy presents a moderately distorted morphology. A central, bright, yellowish core is evident. Extending outwards from this core is a fainter, bluish plume-like structure. This suggests ongoing star formation or a tidal interaction. The galaxy's overall shape is neither perfectly elliptical nor spiral, leaning towards a somewhat irregular form. There may be evidence of minor disturbances or a past merger event, given the asymmetric light distribution and plume extending away from the central region. Further spectral analysis is needed to determine the composition and nature of the plume, and to confirm the presence of tidal features or star-forming regions.
