The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that dominates its morphology. Its overall shape approximates a rounded form, though with a slight ellipticity. The color profile suggests a population of older stars, indicated by a yellow hue, concentrated within the bulge. There is limited evidence of spiral arm structure or significant ongoing star formation activity. The galaxy appears undisturbed, lacking any prominent signs of recent merger events or tidal interactions. There are some very slight blue colors visible in the halo, perhaps indicating that some star formation is occuring. Overall, the observed characteristics suggest an evolved galaxy, potentially a lenticular galaxy, with a well-established stellar population and minimal ongoing star formation.
