The galaxy presents an elliptical morphology, appearing largely smooth and without prominent spiral arm structures. Its shape is somewhat elongated, resembling an ellipse that is moderately cigar-shaped. The galaxy exhibits a central bulge that is bright and concentrated. The color profile suggests that it is dominated by older stellar populations, indicative of relatively low levels of recent or ongoing star formation. There's no visible evidence of active merging events or major disturbances to the overall structure. There are some small distortions that might represent minor disturbances.
