The galaxy presents a relatively smooth, elliptical morphology. It appears largely spheroidal in shape with a high degree of central concentration. There is a bright, yellowish core that fades outwards. Faint extensions or arms are not visible. The galaxy lacks obvious spiral structure or significant dust lanes. The color profile suggests a predominantly older stellar population, although some bluer regions are present. There is no strong indication of ongoing major merging activity or tidal disturbances, although slight asymmetry could suggest a minor interaction or internal dynamic process. The galaxy appears somewhat compact with an approximate effective radius of 4 kpc.