The galaxy appears as a centrally concentrated, elliptical-like structure. It displays a smooth, gradual falloff in surface brightness from the core outwards. The central region is bright and exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the center, the color appears to slightly shift towards redder tones, with a very faint hint of blue possibly present in the outer regions. There are no distinct spiral arm features or dust lanes visible. The overall shape approximates a rounded form, though it could potentially be an inclined disk galaxy, or a spheroid. There is no obvious evidence of any major ongoing merger activity, although the structure could be slightly disturbed. The inferred diameter of the galaxy is approximately 7 kpc. The estimated mass of the galaxy is large. The rate of star formation is low.
