Analysis of the galaxy reveals a relatively smooth, centrally concentrated elliptical morphology. There is an absence of any prominent spiral arm structure or significant dust lanes. The galaxy's light profile is dominated by older stellar populations, exhibiting a reddish hue that indicates a low rate of ongoing star formation. The overall symmetry suggests the galaxy is not currently undergoing a major merger event, although subtle irregularities in its outer regions may indicate minor gravitational interactions or tidal disturbances. The galaxy appears to be well evolved, likely a massive system residing at a considerable distance.
