The galaxy appears as a moderately distant object, exhibiting a largely smooth morphology with a slight central concentration of light. The shape is generally elliptical, leaning towards a more circular form, with no discernible spiral arm structures or significant distortions. The color profile suggests a population of older stars, as indicated by the reddish-yellow hue, particularly concentrated in the core. There are no strong indicators of ongoing major star formation within the galaxy, although a faint blue tinge in the outer regions could potentially indicate some low-level star formation activity. The galaxy doesn't seem to be undergoing any major merging activity. There are also no obvious signs of tidal tails or other disturbances that may occur.