The galaxy presents as a primarily smooth object, with a concentrated central region.  It exhibits a slightly elongated, in-between roundness, deviating from a perfectly spherical shape but not markedly cigar-shaped. The color profile suggests a moderate population of older stars, trending towards redder wavelengths, alongside a population of younger, bluer stars. There is evidence of a minor interaction or disturbance in the galaxy's morphology, given its irregularities. The galaxy appears to be undergoing a merger. It's likely a low-mass system with moderate quenching of star formation.
