The galaxy presents an elliptical morphology, appearing generally smooth with a high degree of central concentration. Its shape is elongated, exhibiting a moderate cigar-shaped profile. The color gradient indicates a population of older stars, contributing to its overall yellowish hue. There's no clear evidence of ongoing major mergers, though subtle disturbances or minor interactions cannot be entirely ruled out based on this image alone. The galaxy possesses substantial mass, inferred from its luminosity, and exhibits relatively low current star formation activity. The overall structure suggests it is a relatively evolved system.
