The galaxy presents as a generally smooth structure with a slight, but noticeable, deviation from perfect sphericity. It appears to be moderately rounded, transitioning from a round shape towards a more elongated form. The galaxy displays a central concentration of light, suggesting a prominent bulge or nucleus. There is some evidence of possible interaction or disturbance in the galaxy's overall morphology, with a possible faint tidal feature or asymmetry visible, but this is uncertain. This galaxy has an approximate diameter of 5.8 kpc.

The galaxy exhibits a colour gradient, appearing bluer towards the outer regions and redder in the central core. This could indicate a younger stellar population in the outer disk or ongoing star formation, with older, redder stars concentrated in the bulge. The overall luminosity suggests that this galaxy is a moderately luminous object.
