The galaxy appears as a centrally concentrated object with a generally smooth morphology. The galaxy exhibits a slightly elongated, but roughly circular shape. There's a dominant central bulge that is bright and relatively unresolved, surrounded by a fainter and bluer, disk-like structure. This suggests a substantial population of younger, bluer stars contributing to the outer regions. There is a slight suggestion of faint spiral arms or tidal disturbances, indicating possible interactions with other galaxies or recent merger activity. The redder central color might indicate the presence of an older stellar population. There appear to be low levels of star formation occurring, inferred from the blue color in its outer regions. Overall, the galaxy presents a complex structure indicative of both evolved and ongoing galactic processes.
