The galaxy appears to be an elliptical type, exhibiting a generally smooth and featureless morphology. The light distribution suggests a centrally concentrated brightness profile, with a gradual decrease in intensity towards the outer regions. The core exhibits a yellowish hue, possibly indicating an older stellar population. There is minimal evidence of spiral arms or prominent dust lanes. The galaxy displays a slight elongation in shape, with an aspect ratio that deviates somewhat from perfectly circular. There is no obvious sign of tidal interactions or ongoing major merger events, although there is a slight hint of asymmetry in its outer regions.
