The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. Its overall shape is roughly round, with a slight deviation towards an intermediate ellipticity. The central region is characterized by a concentrated, bright core that diminishes gradually into the outer regions. There is no obvious presence of a prominent disk structure or spiral arms. The color profile suggests an older stellar population, with a subtle trend toward redder hues. There is no indication of major disturbances, such as tidal tails or disrupted morphology, suggesting it is likely not undergoing a major merging event. Minor irregularities might be present but the images quality limits any definitive assessments.
