The galaxy presents a generally elliptical morphology. It appears largely smooth, with a highly concentrated central bulge dominating the overall luminosity profile. The light distribution suggests a relatively even stellar population, and the galaxy has a color profile indicating an older stellar population. There is no clear evidence of spiral arms or a prominent disk structure. Minor irregularities may be present in the outer regions, but it appears to be overall undisturbed. There is no obvious sign of active star formation.
