The galaxy presents a generally elliptical morphology, with a high degree of central concentration. The light profile appears relatively smooth, indicating a lack of prominent spiral arms or strong dust lanes. The central bulge is quite pronounced and exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the center, the galaxy exhibits a gradual decrease in surface brightness. The outer regions appear more diffuse and slightly bluer in color, hinting at the presence of some younger stars, although this is not as prominent as in typical spiral galaxies. The galaxy's overall shape indicates that it is an elliptical galaxy viewed somewhat close to edge-on. There is no evidence of any significant tidal disturbances or interactions with other galaxies. The light distribution is quite regular.
