The galaxy presents as a relatively compact object with an apparent smooth morphology. The central region exhibits a somewhat higher surface brightness concentration, suggesting a possible bulge structure. There is a slight elongation, deviating from a perfectly circular form. The overall color appears somewhat redder, implying an older stellar population or possible dust attenuation. Faint hints of spiral structure may be present, though these are not prominently defined. No obvious signs of ongoing major mergers or tidal disturbances are evident in the immediate vicinity. The galaxy is likely a disk galaxy, seen at a moderate inclination. The light indicates recent star formation. 
