The galaxy exhibits a pronounced elliptical morphology, with a high degree of elongation. The light distribution suggests a relatively smooth profile, with a higher concentration of light toward the galactic center. There is evidence of disk-like features. The color gradient appears to shift from redder hues in the central bulge to bluer tones in the outer regions, suggestive of recent or ongoing star formation activity in the outer arms. There is slight evidence of a minor tidal disturbance.
