The galaxy presents as a largely featureless, elliptical or spheroidal structure. Its morphology is predominantly smooth, with a high degree of central concentration indicated by the bright central region, which gradually diffuses outward. The overall shape appears round, lacking any significant elongation or asymmetry. There is no visual evidence of prominent spiral arms, bars, or significant dust lanes. The color profile suggests a population of older stars, exhibiting a somewhat redder hue than might be expected in actively star-forming regions. Overall, this galaxy appears to be a relatively quiescent system with little ongoing star formation, likely composed of an older stellar population.
