The galaxy presents a generally elliptical morphology, though with some indications of structural disturbance. There appears to be a central, luminous bulge region with a yellowish hue, suggesting an older stellar population. Extending outwards from the bulge, fainter, more diffuse structures are observed. These structures appear less uniform and exhibit a bluer color, hinting at ongoing star formation. The galaxy shows evidence of interaction or merger activity, possibly with a smaller companion. There is the potential that what appears as a companion could be one of its spiral arms disrupted by an outside force. Overall, the galaxy’s color profile suggests a mix of evolved and actively forming stellar populations, indicative of a complex evolutionary history.
