The galaxy appears to be a spheroidal object, exhibiting a high degree of central concentration. Its light profile appears relatively smooth, showing little in the way of distinct features such as spiral arms or prominent dust lanes. The galaxy's overall color seems to be on the redder side, suggesting an older stellar population, with star formation having largely ceased. There is a slight elongation, but it is predominantly round in shape. There is no noticeable evidence of any major merging events or significant tidal disturbances within the immediate vicinity. The galaxy appears relatively isolated and undisturbed.
