The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, exhibiting a high degree of roundness. The light profile suggests a lack of prominent spiral arms or distinct disk features. There may be a hint of very slight disturbance, although it appears to be a well-formed galaxy, it does not seem to be merging with another galaxy or significantly disrupted by tidal interactions. The galaxy exhibits a color gradient, transitioning from a central core of yellowish-white light outwards to a reddish-hue, potentially indicating a population of older stars in the outer regions. The relatively compact size indicates that the light is emanating from a localized and somewhat compact region. Star formation is likely occurring at a lower rate within this galaxy. Its overall appearance suggests a significant stellar mass and high luminosity.
