The galaxy appears to be a relatively smooth, elliptical system exhibiting a moderate redshift. Its color profile suggests a population of older stars, with a redder hue dominating the overall light. There is little evidence of significant dust lanes or active star formation regions within the visible spectrum. The galaxy's shape is generally round, with a slight deviation towards an intermediate elliptical form. There are no obvious signs of major mergers or significant tidal disturbances influencing its structure. The galaxy's morphological classification leans toward a smooth, spheroidal form with minimal features or disk-like components.
