The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular classification. There is a subtle elongation visible, with the galaxy appearing cigar-shaped. The color profile is dominated by warmer tones; the central region exhibits a yellowish-orange hue, indicative of an older stellar population and potentially dust obscuration. Faint blue hints, possibly arising from younger stars, are observed near the periphery. Based on the overall appearance, there is no evidence of a major ongoing merger, though a possible minor disturbance may be present. The galaxy appears relatively isolated with no obvious tidal features or companion galaxies within proximity. It's overall appearance is relatively undisturbed.
