The galaxy presents as a relatively compact object with a centrally concentrated morphology. The color profile suggests a higher intensity in the green channel, potentially indicating strong emission lines indicative of active star formation or an Active Galactic Nucleus. There's a suggestion of a slight disk-like structure viewed nearly edge-on, or a central bar like feature, bisecting the galaxy's core, indicated by a slight elongation. While the galaxy appears largely smooth, subtle irregularities in its outer regions hint at possible tidal disturbances or minor interactions. Overall, the galaxy does not appear to be undergoing a major merger event, but there are subtle features suggesting potential interactions with smaller objects in the past. The light is heavily skewed to the blue end of the spectrum.
