The galaxy presents as a slightly elongated, roughly elliptical object. It is dominated by a bright, concentrated central region, suggesting a substantial nucleus. Surrounding this core is a fainter, more diffuse halo that appears uneven and somewhat clumpy, hinting at potential substructure. The color profile of the galaxy indicates bluer hues in the outer regions, possibly indicative of ongoing star formation there. There is a subtle indication of possible tidal disturbances or interactions with other galaxies that might be responsible for its clumpy appearance. The overall impression is of a galaxy that is not perfectly smooth or symmetrical, with evidence suggesting recent or ongoing activity.
