This galaxy presents a somewhat amorphous appearance. It is elongated, with a central region of higher luminosity and a diffuse halo. The color profile suggests the presence of older stellar populations, with a hint of blue star formation possibly occurring. There is evidence of potential disturbance or irregularity in the galaxy's structure, possibly indicative of a past or ongoing interaction or merger. A portion of the galaxy appears smoother than other portions. The morphological features suggest an intermediate state between a completely smooth, early-type galaxy and a well-defined spiral or disk galaxy.
