The galaxy presents an overall smooth morphology, appearing largely spheroidal in shape. There are some subtle features, possibly suggestive of a disk, but the dominant impression is of a relatively featureless object. The light distribution appears concentrated toward the center, with a diffuse halo extending outwards. There's a slightly elongated structure, hinting at a weak bar or tidal disturbance. Color gradients across the galaxy suggest variations in stellar populations. The central region exhibits a yellowish hue, possibly indicating older stellar populations, whereas the outer regions appear bluer, potentially signifying younger stars or ongoing star formation. The galaxy does not show strong evidence of a major merger, although subtle distortions suggest that minor interactions may have occurred in its past or be ongoing. The galaxy is of intermediate size, larger than a dwarf galaxy but smaller than many large spiral or elliptical galaxies. Overall, it appears to be an evolved system with a moderate amount of star formation and a complex history.
