The galaxy presents a somewhat elliptical morphology, with a prominent, concentrated bulge. The color profile suggests a relatively older stellar population within the bulge, appearing yellow-white. The outer regions of the galaxy exhibit bluer hues, hinting at ongoing star formation or a population of younger, hotter stars in the disk. There's a slight indication of disturbed morphology or faint tidal features extending from the main galactic body, suggesting a possible interaction or recent merger event. The overall structure appears somewhat smooth, but subtle irregularities in the light distribution could be present. Further investigation with higher resolution imaging and spectroscopic data would be required to confirm.
