The galaxy presents as a relatively compact object. Its morphology appears to be predominantly smooth, with a high degree of central concentration. The overall shape is close to round. The color distribution suggests an older stellar population, with a yellowish-orange hue dominating the central region. Fainter, bluer light extends outward from the center, possibly indicating some ongoing, albeit low-level, star formation in the outer regions. No distinct spiral arms or bar structures are discernible. There is no evidence of a major merger or significant tidal disturbances, although very minor irregularities could be present. The object appears to be generally undisturbed.
