The galaxy presents a generally elliptical morphology, appearing relatively smooth and concentrated towards its center. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population likely dominated by red giant stars. The luminosity decreases gradually from the core outwards. Fainter, bluish-green regions are present in the outskirts, hinting at the possibility of some ongoing or recent star formation activity, although this activity appears subdued. There is no clear evidence of spiral arm structures or a prominent disk component in the visible light. The galaxy's overall structure does not exhibit significant signs of major mergers or tidal disturbances. It has a cigar shaped appearance.
