The galaxy presents an overall moderately concentrated profile, though it is not perfectly smooth. The central region appears brighter and more compact, with a gradual decrease in intensity towards the outer edges. The shape is somewhat elongated, appearing more "in between" rather than perfectly round or cigar-shaped. There is evidence of potential disturbances or interactions. There are some indications of possible merging events and some disk-like features are observed. The galaxy exhibits a range of colors. Some regions display a bluer hue, potentially indicating areas of active star formation. Other regions show a redder color, possibly associated with older stellar populations or dust. The overall color suggests a galaxy with an intermediate level of star formation.
