The galaxy presents a generally elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter, bluish extensions are observed along the major axis, hinting at the presence of younger stars and potential star-forming regions, though these features are not prominent. Overall, there is no strong evidence of significant disk structures, spiral arms, or ongoing major mergers based on visual inspection. The apparent shape is elongated, being more "in between" a cigar shape and a rounded shape. Weak disturbances may be present.
