The galaxy presents as a moderately luminous, centrally concentrated object. Its morphology appears to be generally smooth, with a slight elongation suggesting an oblate spheroidal shape. The galaxy's color profile indicates a population of primarily older stars, as evidenced by its redder hue. There is no distinct disk component visible, nor is there evidence of strong spiral arm structure. Some regions of the galaxy show a slightly mottled texture, potentially indicating areas of ongoing or recent minor star formation, though it is faint. The galaxy's overall appearance is consistent with that of an elliptical or S0 type galaxy at moderate redshift, with a mass range placing it within the upper end of average. There are no major distortions or tidal features observed in the immediate vicinity that would suggest a recent major merger event, although some subtle irregularities may indicate minor disturbances. A relatively high degree of internal uniformity is observed.
