The galaxy presents as a somewhat amorphous structure with a notable central concentration of light. There is a relatively smooth distribution of light, suggesting an evolved stellar population. The galaxy appears to be in a possible merging state or in the later stages of a past merger, with evidence of tidal features or minor disturbances in its outer regions. The object exhibits a slightly elongated morphology, not perfectly spherical, but also not exhibiting a highly defined disk structure. There is a suggestion of ongoing star formation activity within the galaxy, as indicated by the presence of bluer regions.