The galaxy presents as a moderately bright, slightly elongated object. Its color profile skews toward the bluer end of the spectrum, suggesting a population of younger, hotter stars. There is a definite smoothness to its overall appearance, with a hint of disk structure. There's potential evidence of a minor disturbance or interaction, possibly an ongoing merger event, that may be responsible for the feature. Based on color gradients and general morphology, this galaxy exhibits a suppressed star formation rate compared to its mass, indicating it is likely a relatively evolved system, perhaps in transition.
