The galaxy presents a slightly elliptical morphology, appearing more disc-like than spheroidal. Its core exhibits a prominent yellowish hue, suggesting a population of older, redder stars. The outer regions are less defined, fading into a faint bluish halo that could indicate some ongoing star formation. There is slight visual evidence of possible minor disturbances to the morphology. Overall, the galaxy appears relatively compact with an estimated diameter of approximately 7 kpc. Its estimated mass appears to be around 10^10 solar masses, with a relatively moderate star formation rate and a relatively low specific star formation rate.
