The galaxy presents a morphology consistent with an elliptical type, exhibiting a relatively smooth light distribution. There is little evidence of spiral arm structures or significant dust lanes. Its light profile appears concentrated, with a high degree of central symmetry and a round shape. There is some evidence that it may be interacting with smaller objects in its group, implying a potential evolutionary history influenced by mergers or tidal interactions with satellite galaxies. This could be evidence of disturbance to the shape of the galaxy, but there is no major disturbance to the galaxy. Overall, it exhibits characteristics typical of early-type galaxies residing in moderately dense environments.