The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge with a yellowish hue, suggesting a population of older, redder stars. There is a subtle decrease in surface brightness moving outwards from the core, with a faint halo extending beyond the bright central region. There is no apparent dust lane, spiral arm structure, or significant morphological disturbance visible in this image, implying a lack of ongoing major star formation activity. The overall roundness and lack of obvious tidal features indicates that the galaxy has not recently undergone a major merger event. Minor disturbances, such as faint tidal tails or lopsidedness, are not obvious.
