The galaxy appears as a relatively smooth, elliptical-like structure, with a high degree of central concentration. Its overall color is consistent with an older stellar population, exhibiting a reddish hue, suggesting a lack of significant ongoing star formation. The galaxy does not present obvious spiral arm structures or a well-defined disk. There are no signs of a recent major merger or strong tidal disturbances. The galaxy appears fairly isolated and relaxed in terms of morphology, suggesting it may be a lenticular or elliptical galaxy which has used up most of its gas a while ago. The relative lack of blue light indicates that the galaxy is composed primarily of older stars and has a low rate of current star formation.
