The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. Its color profile leans towards the redder end of the spectrum. The galaxy exhibits a relatively high degree of roundness. There appears to be no distinct spiral arm structure or prominent dust lanes. Visual indications suggest a relatively low rate of star formation. There are some indications of minor disturbances to its structure, but it is most likely not undergoing a major merging event.
