The galaxy presents as a moderately bright, somewhat elliptical-shaped object. It appears to possess a dominant central bulge that is relatively smooth and luminous, showing a slightly blueish hue. The light distribution is concentrated towards the center with a gradual decrease in intensity towards the outer regions. A faint, more extended disk structure may be present although indistinct, with the galaxy appearing to have a generally streamlined morphology rather than a distinct spiral structure. There may be some signs of minor disturbances in the galaxy, such as faint tidal tails or an irregular shape in the outer disk. Overall, the galaxy looks like a relatively evolved system with a notable bulge, and moderate star formation rate.
