The galaxy presents as an elongated, cigar-shaped structure. Its morphology appears primarily smooth, with a notable lack of distinct spiral arms or a well-defined central bulge. The light distribution is concentrated towards the center, gradually fading towards the edges. There is some evidence of a faint disk like structure, but it is not dominant, and the overall appearance suggests a galaxy undergoing a transition from a spiral to a more lenticular or elliptical form. The color profile indicates the presence of both older stellar populations contributing to the reddish-yellow hue at the center, and a younger, bluer population towards the outer regions of the disk. There's no apparent presence of active galactic nuclei or significant dust lanes. No signs of major merging events are observed; the overall structure is relatively undisturbed.
