This galaxy exhibits a generally smooth morphology, with a slight elongation. The central region presents a higher concentration of light, suggestive of a prominent galactic bulge or nucleus. The color profile indicates a possible transition from bluer light in the central regions to slightly redder hues in the outer regions, potentially signifying variations in stellar populations and ongoing star formation. There is a faint disk structure present. There's also some evidence of minor disturbance in the galaxy's morphology, which could be caused by a small tidal interaction.
