The galaxy presents as a relatively smooth, elliptical-like object with an apparent shallow inclination relative to our line of sight. Its light is dominated by a central bulge, which appears to be composed primarily of older stellar populations, indicated by the apparent yellow-red color. There's a hint of a more extended disk structure surrounding the bulge, though it lacks prominent spiral arms. The disk appears bluer in color, suggesting the presence of younger, hotter stars, indicating ongoing or recent star formation activity at a low rate. Overall, the galaxy is moderately luminous. There appear to be no signs of any major ongoing mergers or tidal disturbances.
