This galaxy presents as an elongated, smooth structure, appearing cigar-shaped in its overall morphology. The central region exhibits a bright, concentrated luminosity, suggesting a high density of stars or the potential presence of an active galactic nucleus.

Moving outward from the core, the galaxy transitions into a less intensely luminous halo. There's a noticeable blue hue in the outer regions, indicating the presence of younger, hotter stars and ongoing star formation. The smooth appearance and lack of defined spiral arms point towards a relatively evolved system, likely an elliptical or lenticular galaxy with a measurable amount of star formation in the periphery. There is no evidence of any major ongoing merger events, but potentially some minor disturbances in the outer areas of the halo.
