The galaxy presents a morphology that is not clearly defined as purely elliptical or spiral. There is evidence of a central, luminous bulge region which appears approximately smooth in texture. Surrounding this bulge, there is a faint, diffuse disk component that does not exhibit prominent spiral arm structures.

The color profile suggests the presence of both older stellar populations, indicated by the presence of yellow and red hues, particularly towards the central bulge, and areas of more recent star formation, evidenced by subtle blue tones within the disk. Irregularities in the distribution of light suggest potential disturbances in the galaxy's morphology. These disturbances may be indicative of minor gravitational interactions with another galaxy, or internal processes such as active galactic nuclei (AGN) activity. The asymmetry in the distribution of the faint outer regions further hints at a potentially ongoing interaction, perhaps a minor merger event, though no distinct companion galaxy is immediately apparent in this image.
