The galaxy appears as a centrally concentrated object with a smooth light distribution, suggesting a lack of significant spiral arm structure or prominent dust lanes. It exhibits an elliptical morphology, appearing moderately rounded rather than highly elongated or cigar-shaped. The galaxy's color profile indicates a relatively evolved stellar population, trending towards redder hues. There is no obvious indication of ongoing major merging activity, although some minor disturbances may be present. Overall, the galaxy presents as a well-established system with characteristics typical of elliptical galaxies at the observed redshift.
