The galaxy presents as a centrally concentrated object with a generally smooth morphology. The primary color is a blend of yellow and white, suggesting a stellar population dominated by older stars, likely in the galactic bulge. There is a slight elongation, hinting at either a disk-like structure or potential tidal disturbance, but the smoothness suggests it is unlikely to be a spiral galaxy. The absence of distinct spiral arms or knots of star formation implies a relatively low star formation rate. A hint of blue-ish color extending along the elongated axis could indicate the presence of younger stars within the apparent disk. There is no clear evidence of a major merger, but some minor disturbances or interactions may be present based on the slight asymmetry.
