The galaxy presents a largely smooth morphology, appearing somewhat spheroidal in shape. A distinct central bulge is visible, characterized by a high surface brightness and a yellowish hue. There is no apparent disk structure, nor are there any clear spiral arms. The galaxy exhibits a relatively compact appearance, with a diameter estimated to be approximately 5 kpc. The outer regions of the galaxy appear less defined and more diffuse compared to the central bulge. Based on the observed color profile, the galaxy appears to be primarily composed of older stellar populations. There is no sign of active star formation or recent merger events. The galaxy's structure appears relaxed, showing little evidence of significant gravitational disturbance or interaction with neighboring galaxies.
