The galaxy presents as a moderately bright object with a predominantly smooth morphology. Its overall shape appears somewhat rounded, though not perfectly spherical. There is a suggestion of internal structure, but it is subdued, lacking prominent spiral arms or a distinct bar. The central region exhibits a concentrated brightness, potentially indicating the presence of a bulge. The light distribution suggests a mature stellar population. There is evidence of ongoing star formation, as indicated by the slightly bluer hues in the galaxy’s overall color. There may be minor disturbances present, although no clear signs of a merger in progress are obvious.
