The galaxy presents an overall smooth appearance, though with some suggestion of structure within. The central region appears brighter and more condensed, with a somewhat irregular shape exhibiting subtle color variations. There is a slightly elongated morphology, not perfectly spherical but neither highly flattened or cigar-shaped. The light distribution suggests a moderate amount of internal disruption or merging activity in its recent history. Star formation appears to be present, but it's likely at a moderate rate given the colors observed.
