The galaxy presents as a cigar-shaped, elongated structure, suggesting it is an elliptical galaxy viewed at an angle. Its central region exhibits a yellowish hue, potentially indicative of an older stellar population dominating the core. Moving outward from the center, a gradual color transition occurs towards the edges, showing some bluer tones, hints of ongoing, low levels of star formation. No spiral arms or distinct dust lanes are visible; the galaxy appears to be a relatively smooth distribution of stars, lacking prominent features. There appears to be no signs of any ongoing major merging events or tidal disturbances affecting its overall form.
