The galaxy presents an elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures or a distinct disk. It exhibits a centrally concentrated luminosity profile, with the brightest region residing at the core. The galaxy's color gradient suggests an older stellar population is dominant, with a yellow-red hue becoming more pronounced toward the center. A faint, extended halo surrounds the central body, gradually fading into the background. There is little evidence of ongoing major merger activity or significant tidal disturbances, though subtle irregularities may indicate minor interactions in its past. Overall, the galaxy appears to be a relatively quiescent system, consistent with a more evolved state.
