The galaxy presents a predominantly smooth and elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The overall shape is elongated, exhibiting a cigar-like appearance rather than a perfect sphere or disk. There are some suggestions of a slight disturbance in the structure but no clear evidence of any major ongoing merger events or significant tidal features disrupting its form. Color gradients are subtle, with a slightly redder hue in the central regions compared to the outer areas. This suggests a population of older stars dominating the central regions, while the outer regions potentially harbor younger stellar populations or dust. The galaxy shows moderate star forming properties.
