The galaxy presents as an elliptical morphology, elongated in shape, resembling a cigar, but with the ends slightly rounded. The color profile is characterized by a prominent central bulge with a yellow-orange hue, suggesting an older stellar population. The disk surrounding the bulge is less defined, gradually fading outwards. There is no clear evidence of spiral arm structure or dust lanes within the observable portion of the galaxy. Faint traces of blue tinge are visible in the outer regions, hinting at some ongoing, albeit low, star formation activity. Overall, the galaxy exhibits a smooth appearance, with no indications of significant merger events or major disturbances.