The galaxy appears as a single, relatively smooth object with a concentrated central bulge. The overall shape is generally elliptical, showing a high degree of roundness with only a slight deviation towards an elongated form. There is no clear evidence of spiral arms or significant disk structure. The light distribution is largely uniform, with a gradual decrease in intensity from the core outwards. There is a possible minor distortion or disturbance in the overall structure. The color index indicates a redder hue, suggesting an older stellar population. Star formation is likely suppressed, with a low current rate. The estimated size is several kiloparsecs, typical of dwarf galaxies.
