The galaxy presents a moderately elliptical morphology. It appears largely smooth in texture, with a concentrated, bright central bulge that transitions gradually into a fainter, more diffuse halo or disk. The color profile suggests a population of older stars, indicated by the redder hues, particularly in the central region. There is some evidence of bluer star formation regions within the disk, although these are relatively subdued. The structure displays no obvious signs of major disturbances or mergers, though subtle asymmetries cannot be entirely ruled out. Overall, it presents as a fairly evolved system.
