The galaxy appears to be an elliptical galaxy. Its morphology is generally smooth and featureless, with a concentrated central bulge. The light distribution appears to be more elongated than circular, possibly cigar-shaped. The galaxy displays a yellow-orange hue overall, which suggests an older stellar population with less ongoing star formation and a higher proportion of evolved stars. There is no apparent spiral structure or active star-forming regions. No signs of significant tidal disturbances or ongoing major mergers are visually apparent. There may be a minor perturbation, but it is very subtle.
