The galaxy presents a generally smooth and rounded morphology. There is evidence of a central bulge region with a higher concentration of light. The outer regions of the galaxy appear less defined, fading gradually into the background. The color profile suggests a galaxy with a mix of stellar populations, with a slightly yellower hue in the central region. There is a hint of some bluer light around the edges, potentially indicating areas of more recent star formation. However, the smooth overall appearance suggests that star formation rates may be relatively low at present. There are some possible disturbances and/or subtle irregularities in the distribution of the light, which could indicate that this galaxy has undergone a minor merger event in the past.
