The galaxy presents a generally smooth and rounded morphology, with a hint of a disk-like structure. The central region exhibits a bright, concentrated core, potentially indicative of an actively star-forming region or the presence of an active galactic nucleus. There may be indications of some internal structure, although the resolution limits a more detailed assessment. The color profile suggests a mix of stellar populations, with a tendency toward a redder hue, especially in the outer regions. There is no visible evidence of any significant interactions or major disturbances, suggesting a relatively quiescent state. A slight asymmetry exists, leaning toward a cigar shape.
