The galaxy appears as a moderately luminous, elongated structure. Its morphology is generally smooth, with a hint of a disk-like component and no obvious spiral arm features. The central bulge appears to be the brightest region of the galaxy. The color distribution is relatively uniform, with a slightly redder hue in the central regions and a bluer tint extending outwards, potentially indicative of ongoing, but low levels of star formation within the galaxy. There is no prominent evidence of tidal disturbances, major mergers, or other significant morphological irregularities. The overall appearance suggests a galaxy that is somewhere on the transition between spiral and elliptical.
