The galaxy appears to be a relatively compact, elliptical system at a redshift of approximately 0.24. It exhibits a smooth, fairly spherical morphology with no apparent spiral arm structures or significant dust lanes. The central region shows a concentrated luminosity, indicative of a prominent galactic nucleus. Faint, diffuse light extends outwards from the core, gradually fading into the background. The galaxy exhibits a slightly bluer color profile in the central region, shifting to redder tones in the outer edges. There is no obvious evidence of ongoing major mergers or tidal disturbances in this image. The overall appearance suggests a system dominated by an older stellar population. Based on its color and smooth features, it appears to be a relatively massive galaxy with moderate star formation rates.
