The galaxy presents as a somewhat concentrated, moderately luminous object. It exhibits a slight elongation, deviating from a perfectly circular morphology, but not to the extent of a highly flattened disk. The color profile suggests a diverse stellar population, with a central, somewhat bright, yellow region indicative of older stars, surrounded by fainter, blue clumps, possibly indicating pockets of recent or ongoing star formation. There is some indication of disturbances to the galaxy which could mean the presence of a merging galaxy in the background. There appears to be a slightly uneven luminosity distribution across its body, suggesting the possibility of minor disturbances.
