The galaxy presents as a relatively compact object with a slightly elongated morphology. The color profile suggests a mix of stellar populations, with a dominant yellowish-orange hue concentrated towards the galaxy's core, possibly indicating older, redder stars. Fainter, bluer regions appear scattered throughout, hinting at some ongoing or recent star formation activity. The overall structure lacks a clearly defined spiral arm pattern, but subtle irregularities and faint extensions suggest the presence of tidal features or disturbances. The galaxy appears to be a relatively massive system and may be undergoing a minor interaction or merger event, although a smooth morphology seems to be dominating. Star formation activity appears to be on the low side.
