The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is evidence of a slight elongation, presenting an intermediate roundness rather than a perfectly spherical shape. Subtle irregularities are visible, suggesting the possibility of minor disturbances. The color gradients transition from bluer hues in the central region to redder tones towards the outer edges, potentially indicative of varying stellar populations. The overall structure does not exhibit characteristics typically associated with major mergers. A subtle extension or tidal feature may be present, requiring further investigation to determine its origin and association with the galaxy.
