The galaxy presents as a relatively compact object, approximately 8.2 kpc in diameter, exhibiting a largely smooth morphology with a centrally concentrated luminosity. The central region displays a slight reddish hue, potentially indicative of an older stellar population or dust obscuration. There is a faint disk visible that is not very pronounced. The surrounding galactic halo appears relatively uniform in color, though there may be some slight disturbances indicative of minor gravitational interaction. There is no evidence of a significant merger event occurring in the recent past. The galaxy exhibits an elliptical shape, leaning towards a more spherical structure rather than a highly elongated or cigar-shaped one. Star formation appears to be relatively low.
