The galaxy appears as a roughly elliptical, yet asymmetric, structure with a centrally concentrated luminosity profile. The color distribution is relatively uniform across the galaxy's visible extent, with a slight suggestion of bluer tones at the periphery and redder tones in the central bulge. The morphology suggests a transition between a classical elliptical galaxy and a disk galaxy, as there is some suggestion of a flattened structure but no distinct spiral arms. There are signs of minor disturbances within the galaxy, indicating possible past or ongoing merger activity. This disturbance does not appear large enough to disrupt the overall structure, but could be affecting star formation within the disk. Overall, the galaxy is moderately luminous.
