The galaxy presents an elliptical morphology, appearing elongated in shape, potentially cigar-shaped, rather than a circular or spiral structure. It exhibits a relatively smooth overall texture with no distinct features. There is no apparent evidence of significant ongoing mergers or major disturbances, though the image resolution limits detailed assessment. The color profile tends toward the redder end of the spectrum, suggesting an older stellar population and potentially lower levels of recent star formation activity, thus possibly resulting in a larger mass. The galaxy size is consistent with previously observed galaxies at similar distances.
