The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. It is elongated, with a cigar-shaped appearance. The color profile suggests a dominant older stellar population, indicated by the yellowish-white hue concentrated in the central region. There is a slight color gradient from the center to the outer regions, which show hints of bluer light, potentially indicating pockets of more recent, though subdued, star formation. Some evidence of minor gravitational disturbance can be seen, though the overall structure appears to be stable. No clear signs of spiral arms or a prominent disk are apparent. The object appears relatively isolated, with no clear indication of a major merger event in progress.
