The galaxy presents as a cigar-shaped, elongated structure with a moderately smooth appearance. There's a distinct central bulge exhibiting a yellowish hue, indicating a population of older stars. Moving outwards from the core, the color shifts to a bluer tint, hinting at the presence of younger, hotter stars within what may be a galactic disk, although any spiral arm structures are indistinct from this view. The overall morphology suggests that this is likely an elliptical or lenticular galaxy, with a preference toward the elliptical type due to its lack of defined spiral arms and the notable elongation. It appears to be a relatively massive galaxy, exhibiting quiescient star formation characteristics. There is no obvious evidence of major merger activity. The relative smoothness and redder color towards the center suggest that the majority of star formation is likely suppressed.
