The galaxy appears to be a relatively smooth, elliptical type galaxy, likely at an intermediate redshift. Its light distribution is concentrated towards the center, with a gradual decrease in intensity outwards, showing no distinct spiral arm structures or features. The galaxy's light is somewhat red, which could be due to a combination of factors including its intrinsic stellar population being dominated by older, redder stars, and/or redshift effects. There is no evidence of ongoing major mergers or significant tidal disturbances. There may be some minor internal structure but it is blurred and ill defined.