The galaxy presents as a centrally concentrated object with a smooth, diffuse profile. The light distribution appears relatively even across the main body of the galaxy, with no distinct spiral arm structures or prominent star-forming regions visible. It exhibits an elliptical morphology, elongated along one axis, resembling a cigar shape. The galaxy's core displays a yellowish hue, possibly indicating an older stellar population. Fainter, bluer light is seen extending from the center, potentially hinting at some level of ongoing star formation or a population of younger stars within the disk. There is no indication of any major mergers or significant tidal disturbances in its appearance, but there are subtle features that could suggest minor disturbances or interactions. The galaxy’s overall structure appears relatively undisturbed.
