The galaxy presents a predominantly smooth morphology, exhibiting a concentrated central region. Its shape is moderately elliptical, showing a deviation from a perfect circular appearance. There is no clear evidence of a prominent disk structure or spiral arms. Minor disturbances are present, hinting at a possible past interaction or merger event. The galaxy displays a moderate level of star formation activity.

The color profile suggests a population of relatively old stars. The galaxy appears to have an approximate effective radius of 3.7 kpc. Overall the galaxy appears to be a relatively massive system.
