The galaxy presents as a relatively compact, elliptical-like structure with a high degree of central concentration. Its light profile is smooth, lacking any prominent spiral arms or distinct morphological features. The core of the galaxy is bright, suggesting a high stellar density or possible AGN activity. There is some elongation to the galaxy's shape, transitioning from round, but it isn't elongated enough to be cigar-shaped. Some visual distortion could indicate a past or ongoing minor interaction.
